3131/2=============================================================== HD 26 BD +07 5128 G4V:P (CH, EMISS H+K) AR 00 02.8 DEC +08 31 MV = 8.22 FE/H = - R ------------------------------------------------------------------------ ( 18) WALLERSTEIN, G., GREENSTEIN, J.L. 1964: ASTROPHYS.J. 139, 1163 ........................................................................ OBSERV. : PG, 4380-4600A, 9 A/MM, 5165-6800A, 6.7-13.5 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(EPS VIR), T(BVGRI) REMARKS : CH-STAR COMMENTS: BEFORE REVISION OF FE F-VALUES CLASS : DTAA, (I) ------------------------------------------------------------------------ (A30) LUCK, R.E., BOND, H.E. 1982: ASTROPHYS.J. 259, 792 ........................................................................ OBSERV. : PG, 3800-5000A, 9 A/MM; 50A SECTIONS IN 5100-7800A, 0.2A, S/N= 30..50 (RETICON) INSTRUM.: MT.PALOMAR 200-INCH; MT.WILSON 100-INCH, COUDE, RETICON LINELIST: 180: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 611 BD +59 5 G2IB-II AR 00 08.0 DEC +60 32 MV = 8.20 FE/H = - (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 886 GAM PEG B2IV (BET CEP) AR 00 10.7 DEC +14 54 MV = 2.83 FE/H = 0 R ------------------------------------------------------------------------ (187) SNIJDERS, M.A.J. 1969: ASTRON.ASTROPHYS. 1, 452 ........................................................................ OBSERV. : PG, 4081-4313A, 5-11 A/MM INSTRUM.: DAO LINELIST: LW, 6 ANALYSIS: LTE(UNDERHILL), T+G(UNDERHILL 1968: VISTAS ASTRON. 8, 41) F-VALUES FROM WARNER(1965), COMPARES SOME LINEPROFILES REMARKS : 6 FE-LINES COMMENTS: PRE-UV CLASS : MA ------------------------------------------------------------------------ (375) PETERS, G.J. 1976: ASTROPHYS.J. SUPPL. 30, 551 ........................................................................ OBSERV. : PG, 3090-6700A, 2 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 274 ANALYSIS: LTE(MORTON), T+G(SCAN 1400-8100A, HGAMMA+HDELTA, SI III/IV + SII/III IONIZATION) REMARKS : CALC. LINE-BLANK. SHORTWARD OF 2200A WEAKER THAN OBS. COMMENTS: CLASS : TGMAA, R ======================================================================== HD 1326 GJ 15A M1V (EMISS H+K) AR 00 15.5 DEC +43 44 MV = 8.09 FE/H = - (L) ------------------------------------------------------------------------ (313) MOULD, J.R., 1978: ASTROPHYS.J. 226, 923 ........................................................................ OBSERV. : 1.5-2.5 MU, 1.5 A (= 4000-6600CM**-1, 0.3 CM**-1) INSTRUM.: KPNO 4M, FTS LINELIST: LW, 22 ANALYSIS: LTE(MOULD 1976), SPECTRUM SYNTHESIS, T(7540-10175 COLOUR), F-VALUES: DIFF(SUN), THEORETICAL VALUES REMARKS : METALLICITY FROM AL, CA, MG COMMENTS: CLASS : (D)TMSA, (L) ======================================================================== HD 1461 HR 72 G0V AR 00 16.1 DEC -08 20 MV = 6.46 FE/H = 0 R ------------------------------------------------------------------------ ( 74) SPINRAD, H., LUEBKE, W.R. 1970: ASTROPHYS.J. 160, 1141 ........................................................................ OBSERV. : PG, 5180-5880A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(COLOUR 5360-7400A) REMARKS : SUPER-METAL-RICH COMMENTS: CLASS : DTA, L ------------------------------------------------------------------------ (128) BRANCH, D., BELL, R.A. 1971: MONTHLY NOT.ROY.ASTRON.SOC. 153, 57 ........................................................................ OBSERV. : PG, 5200-6240A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 262 ANALYSIS: THEOR.COG, T(COLOUR 5360-7400A) TEMP-TAU-RELATION: KRISHNA SWAMY 1967: AP.J. 150, 1161 FE F-VALUES: CORLISS(1968) REMARKS : SUPER-METAL-RICH COMMENTS: CLASS : T(M)AA, L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 1581 ZET TUC F9V AR 00 17.5 DEC -65 10 MV = 4.20 FE/H = 0 (L) ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), (L) ======================================================================== HD 1835 9 CET G2V (EMISS H+K) AR 00 20.3 DEC -12 29 MV = 6.38 FE/H = 0 (L) ------------------------------------------------------------------------ (324) CAYREL DE STROBEL, G., KNOWLES, N., HERNANDEZ, G., BENTOLILA, C. 1981: ASTRON.ASTROPHYS. 94, 1 ........................................................................ OBSERV. : PG, 4000-4900A, 12.4A/MM, 0.30A INSTRUM.: OHP 1.52M, COUDE LINELIST: LLWW, 210: ANALYSIS: COG, DIFF(SUN), T(B-Y, B2-V1, HBETA+HGAMMA), G(4383A) REMARKS : LOOKING FOR SOLAR TWINS COMMENTS: CLASS : DTGAA, (L) ======================================================================== HD 2151 BET HYI G2IV (EMISS H+K, FAINT BLUE *) AR 00 23.1 DEC -77 32 MV = 2.80 FE/H = - R ------------------------------------------------------------------------ ( 20) RODGERS, A.W., BELL, R.A. 1963: OBSERVATORY 83, 79 ........................................................................ OBSERV. : PG, ???? , 2.7 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 300: ANALYSIS: COG, DIFF(SUN), T(MK-TYPE) REMARKS : ANALYSIS AS RODGERS 1963, MNRAS 127, 471 COMMENTS: SHORT COMMUNICATION CLASS : DAA ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 2421 HR 104 A2VS AR 00 25.5 DEC +44 07 MV = 5.17 FE/H = 0 (L) ------------------------------------------------------------------------ (145) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 154, 975 ........................................................................ OBSERV. : PG, 3300-6250A, 4.5+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 300: ANALYSIS: LTE(STROM), T+G(FE I EXCITATION, FEI/II IONIZATION) REMARKS : COMMENTS: BVI COLOURS ARE NOT EXPLICITLY COMPARED WITH MODEL COLOURS CLASS : TGMAA, (L) ======================================================================== HD 2490 HR 109 M0III AR 00 26.0 DEC -40 11 MV = 5.44 FE/H = 0 (L) ------------------------------------------------------------------------ (239) WEGNER, G. 1976: MONTHLY NOTICES ROY.ASTRON.SOC. 177, 3 ........................................................................ OBSERV. : PG, 4554-5002A, 6.8 A/MM INSTRUM.: RADCLIFFE 1.9M, COUDE LINELIST: 125 ANALYSIS: COG, DIFF(ALF BOO), T(UBVRI, R-I), PE(TI I/II IONIZATION) F-VALUES FROM ARCTURUS ATLAS(GRIFFIN 1968) REMARKS : COMMENTS: CLASS : DTA, (L) ======================================================================== HD 2665 BD +56 70 G5III (WEAK METALS) AR 00 28.0 DEC +56 47 MV = 7.73 FE/H = ---- L ------------------------------------------------------------------------ ( 42) KOELBLOED, D. 1969: ASTROPHYS.J. 149, 299 ........................................................................ OBSERV. : PG, ??? , 9+14 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR, 300 ANALYSIS: COG, DIFF(SUN), T(COG) REMARKS : EXTREME HIGH VELOCITY STAR COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : DTAA, L ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O KOELBLOED HAS BETTER OBS. DATA COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, L ======================================================================== HD 2796 BD -17 10 G0 (WEAK METALS) AR 00 28.8 DEC -17 04 MV = 8.51 FE/H = ---- R ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA ------------------------------------------------------------------------ (399) BESSELL, M.S., NORRIS, J. 1981: ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS, IAU COLLOQ. NO. 68, A.G.D.PHILIP, D.S.HAYES EDS., L.DAVIS PRESS, SCHENECTADY, N.Y., P. 94 ........................................................................ OBSERV. : PE, ??? 5 A/MM INSTRUM.: AAT 3.9M, IPCS LINELIST: 124 ANALYSIS: LTE(GUSTAFSSON, ATLAS), T(BVRI, DDO, UVBY, CMT1T2), T+G(BVRI, DDO, UVBY, CMT1T2; LINE STRENGTH, EXCITATION, IONIZATION), F-VALUES: ABSOLUTE (FE I: BLACKWELL 1980) MOLEK.BANDS: SPECTRUM SYNTHESIS, F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : TGMAA, R? ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, CTIO 1.5M, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A19) BESSELL, M.S., NORRIS, J. 1984: ASTROPHYS.J. 285, 622 ........................................................................ OBSERV. : SECTIONS AT 3840-5900A, 10+16 A/MM, 0.3+0.6 A, 6-12 SPECTRA COADDED INSTRUM.: AAT 3.9M, IPCS LINELIST: LW, 90 ANALYSIS: LTE(ATLAS, UNBLANKETED; GUSTAFSSON), T+G(TI I,II, FE I,II LINES), SPECTRUM SYNTHESIS FOR NH, CH BANDS F-VALUES: FE I(BLACKWELL, BRIDGES+KORNBLITH) REMARKS : COMMENTS: CLASS : TGMSAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 2857 BD -06 86 A2 (HOR.BRANCH, HALO) AR 00 29.3 DEC -05 32 MV = 10.00 FE/H = --- R ------------------------------------------------------------------------ (379) DANFORD, S.C., LEA, S.M. 1981: ASTRON.J. 86, 1909 ........................................................................ OBSERV. : PG, 4850-4700A, 16.9 A/MM INSTRUM.: KPNO 2.1M, COUDE LINELIST: LW, 46 ANALYSIS: LTE(ATLAS), T+G(SCAN: DANFORD 1976: THESIS, YALE UNIV.) F-VALUES: VARIOUS SOURCES (1969-78) LISTED REMARKS : COMMENTS: CLASS : MAA, L ------------------------------------------------------------------------ (405) KODAIRA, K., PHILIP, A.G.D. 1981: ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS, IAU COLLOQ. NO. 68, A.G.D.PHILIP, D.S.HAYES EDS., L.DAVIS PRESS, SCHENECTADY, N.Y., P. 153 ........................................................................ OBSERV. : ??? 12.5 A/MM ?? INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: ANALYSIS: LTE(ATLAS), T+G(PHOTOMETRY, HDELTA PROFILE) REMARKS : GIVE FE/H ONLY COMMENTS: SUPERSEDED BY (A22) CLASS : TGMA ------------------------------------------------------------------------ (A22) KODAIRA, K., PHILIP, A.G.D. 1984: ASTROPHYS.J. 278, 208 ........................................................................ OBSERV. : PG, 3850-4300A, 12.5 A/MM INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), DIFF(HD 161817), T+G(B-V, C1, M1, HDELTA WING), F-VALUES: KURUCZ+PEYTREMANN 1975 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 3360 ZET CAS B2IV AR 00 34.2 DEC +53 37 MV = 3.66 FE/H = + (I) ------------------------------------------------------------------------ (187) SNIJDERS, M.A.J. 1969: ASTRON.ASTROPHYS. 1, 452 ........................................................................ OBSERV. : PG, 4081-4313A, 5-11 A/MM INSTRUM.: DAO LINELIST: LW, 6 ANALYSIS: LTE(UNDERHILL), T+G(UNDERHILL 1968: VISTAS ASTRON.8, 41) F-VALUES FROM WARNER(1965), COMPARES SOME LINEPROFILES REMARKS : 6 FE-LINES COMMENTS: PRE-UV CLASS : MA, (I) ======================================================================== HD 3369 PI AND B5V AR 00 34.2 DEC +33 27 MV = 4.36 FE/H = 0 (L) ------------------------------------------------------------------------ (331) HEACOX, W.D. 1979: ASTROPHYS.J.SUPPL. 41, 675 ........................................................................ OBSERV. : PG, 3100-4700A, 6.8 A/MM, 0.14 A, MN III (1285 A) INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LLWW, 80: ANALYSIS: LTE(KPA), T(C0,M0), G(HGAMMA, HDELTA) FE F-VALUES OF WARNER(1967), CORRECTED AFTER SMITH(1976) REMARKS : GIVES ABUNDANCES FOR XI = 0 AND 3 KM/S COMMENTS: CLASS : TGMAA, (L) ======================================================================== HD 3443 HR 159 G8V (EMISS H+K) AR 00 34.8 DEC -25 03 MV = 5.57 FE/H = 0 (R) ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : ASSUMES SYSTEM OF TWO IDENTICAL STARS COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 3546 EPS AND G8III (CH) AR 00 35.9 DEC +29 02 MV = 4.37 FE/H = - (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 3627 DEL AND K3III SB (EMISS H+K) AR 00 36.6 DEC +30 35 MV = 3.27 FE/H = 0 R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 3651 54 PSC K0V (EMISS H+K) AR 00 36.8 DEC +20 59 MV = 5.80 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 16.3 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) FINDS METAL ENHANCEMENT OF 0.3 DEX IN SUPERMETALRICH STARS COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 3712 ALF CAS K0IIIA (EMISS H+K) AR 00 37.7 DEC +56 16 MV = 2.23 FE/H = 0 R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 3765 GJ 28 K2V (EMISS H+K) AR 00 38.1 DEC +39 55 MV = 7.36 FE/H = 0 (R) ------------------------------------------------------------------------ (246) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 85 ........................................................................ OBSERV. : PG, EGC, 4650-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE LINELIST: LLWW, 200: ANALYSIS: DIFF(SUN), LTE(PEYTREMANN 1974) T(R-I) G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUND. ONLY COMMENTS: CF. HEARNSHAW 1976: A.A. 51, 71 CLASS : DTGMA ======================================================================== HD 4128 BET CET K0III VAR (EMISS H+K) AR 00 41.1 DEC -18 16 MV = 2.04 FE/H = 0 R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R ------------------------------------------------------------------------ (382) KOVACS, N. 1982: ASTRON.ASTROPHYS. 120, 21 ........................................................................ OBSERV. : PG, 4700-6100A, 3.3 A/MM INSTRUM.: ESO 1.5M LINELIST: LLWW, 415 ANALYSIS: DIFF(SUN), LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19 ) T(UBVRIJK, 52,63,72,80,86) G(FEI/II IONIZATION) REMARKS : FINDS LITTLE EVIDENCE FOR NLTE EFFECTS COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 4306 BD -10 155 G0 (WEAK METALS, FAINT BLUE *) AR 00 42.9 DEC -09 49 MV = 9.02 FE/H = ---- R ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, CTIO 1.5M, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 4362 HR 207 G0IB AR 00 43.8 DEC +59 18 MV = 6.39 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 4382 23 CAS B8III AR 00 44.4 DEC +74 34 MV = 5.41 FE/H = 0 (L) ------------------------------------------------------------------------ (265) ALLEN, M.S. 1977: ASTROPHYS.J. 213, 121 ........................................................................ OBSERV. : PG, 3700-4150A, 4200-4650A, 2.4 A/MM, 0.074A (FWHM) INSTRUM.: DAO 1.2M, COUDE, IMAGE SLICER LINELIST: 66, DAOR ANALYSIS: LTE(KCG 1969), T+G(UBV, HGAMMA, FE I/II IONIZATION) F-VALUES: EXPERIMENTAL, THEORETICAL, SOLAR REMARKS : DERIVES ABUNDANCES FOR FE, SR ONLY COMMENTS: USES STAR AS COMPARISON FOR HG-MN STARS ALLEN, COWLEY 1977: PASP 89, 386 GIVE CR, MN, FE ABUND. CLASS : (D)TGMA, (L) ======================================================================== HD 4395 BD -12 132 G5 AR 00 43.7 DEC -11 44 MV = 7.5 FE/H = - R ------------------------------------------------------------------------ (A30) LUCK, R.E., BOND, H.E. 1982: ASTROPHYS.J. 259, 792 ........................................................................ OBSERV. : PG, 3800-5000A, 9 A/MM; 50A SECTIONS IN 5100-7800A, 0.2A, S/N= 30..50 (RETICON) INSTRUM.: MT.PALOMAR 200-INCH; MT.WILSON 100-INCH, COUDE, RETICON LINELIST: 200 OR MORE ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A29) SNEDEN, C. 1983: PUBL.ASTRON.SOC.PACIFIC 95, 745 ........................................................................ OBSERV. : PE, 50A SECTIONS AT 4230, 4370, 4730 A, 0.3 A, S/N= 100 (D) 95A SECTIONS AT 6325 A, 0.3 A, S/N= 75..200 (RETICON) INSTRUM.: MCDONALD 2.7M, COUDE, DIGICON, RETICON LINELIST: 30: ATOMIC LINES; C2, OI, CH FEATURES ANALYSIS: LTE(ATLAS), SPECTRUM SYNTHESIS FOR MOLECULAR FEATURES, T+G(FROM (A30) LUCK BOND 1982: AP.J. 259, 792: T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION)), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : FINDS LOWER MICROTURBULENCE THAN IN (A30) COMMENTS: CLASS : D(TG)MSA, R ------------------------------------------------------------------------ (A11) KRISHNASWAMY, K., SNEDEN, C. 1985: PUBL.ASTRON.SOC.PACIFIC 97, 407 ........................................................................ OBSERV. : PE, REGIONS BETWEEN 7330-7600 A, 0.1-0.2 A, S/N= 100 INSTRUM.: MCDONALD 2.7M, COUDE, DIGICON LINELIST: LLWW, 250: ANALYSIS: LTE(SNEDEN THESIS 1983), SECTRAL SYNTHESIS, DIFF(SUN, HOLWEGER MODEL), T+G(FE I EXCITATION, FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMSAA, (R) ======================================================================== HD 4539 FB 9 A (SUBDWARF) AR 00 44.9 DEC +09 42 MV = 10.29 FE/H = 0 (L) ------------------------------------------------------------------------ (397) BASCHEK, B., SARGENT, W.L.W., SEARLE, L. 1972: ASTROPHYS.J. 173, 611 ........................................................................ OBSERV. : PG, 3700-5100A, 9+18 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH (9 A/MM), COUDE LINELIST: LLWW, 34 ANALYSIS: DIFF(IOT HER), LTE(ATLAS UNBLANK), T+G(SCAN 3100-5600A, HDELTA+HGAMMA) REMARKS : FIT PROFILES OF HEI 4026+4471 LINES COMMENTS: PRE-UV CLASS : DTGMAA, (L) ======================================================================== HD 4614 ETA CAS G0V SB (EMISS H+K) AR 00 46.0 DEC +57 33 MV = 3.40 FE/H = - R ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3300-4700A, 9+13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y) G(UVBY-BETA, BINARY MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 4817 HR 237 K3IAB: AR 00 48.3 DEC +61 32 MV = 6.07 FE/H = - (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 5015 HR 244 F8V AR 00 50.1 DEC +60 51 MV = 4.82 FE/H = 0 R ------------------------------------------------------------------------ (233) BRANCH, D., BELL, R.A. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 151, 289 ........................................................................ OBSERV. : PG, 3377-4667A, 4.5 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 214 ANALYSIS: COG(SUN), T(BETA) REMARKS : SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713 COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 5544 BD -00 146 K0IIIP: (CN, CH) AR 00 56.7 DEC +00 04 MV = 7.63 FE/H = 0 (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 5780 BD +00 159A K5II-III AR 00 56.8 DEC +00 31 MV = 7.61 FE/H = -- (R) ------------------------------------------------------------------------ (293) FOY, R. 1980: ASTRON.ASTROPHYS. 85, 287 ........................................................................ OBSERV. : PG, 5200?-6200?A, 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(T-TAU FROM GUSTAFSSON) ), T(R-I), G(FE I/II IONIZATION), T+G CHECKED BY: LINE PROFILES OF MG I B TRIPLET F-VALUES AS COMPILED BY FOY 1972: A+A, 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : ABUND. OF ELEMENTS OTHER THAN FE, NA, BA WERE DERIVED FROM WEAK LINES DIFFERENTIALLY TO THE SUN COMMENTS: CLASS : (D)TGMAA, (R) ======================================================================== HD 6268 CD -28 322 G0 (WEAK METALS) AR 01 00.9 DEC -28 09 MV = 8.08 FE/H = ---- R ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A16) BARBUY, B., SPITE, F., SPITE, M. 1985: ASTRON.ASTROPHYS. 144, 343 ........................................................................ OBSERV. : PG, 3800-4950A, 7-10 A/MM, 0.1 A COADDING SEVERAL SPECTRA TO GET S/N= 20..30 INSTRUM.: ESO 1.5M, COUDE, ECHELLE, EGC LINELIST: LLWW, 160: ANALYSIS: LTE(GUSTAFSSON; COG AND LINE-BY-LINE), T(R-I, V-K), G(FE, TI IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL), SYNTHETIC SPECTRA FOR CN, CH, G BANDS REMARKS : COMMENTS: CLASS : DTGMSAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 6497 HR 316 K2III COMP (EMISS H+K) AR 01 04.0 DEC +56 40 MV = 6.43 FE/H = 0 R ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : PG, 4400-6800A, 9.7+12.4 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(EPS VIR), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : COMMENTS: CONFIRMED AND SUPERSEDED BY (165) BECAUSE OF BETTER DATA CLASS : DTGMAA ------------------------------------------------------------------------ (165) CAYREL DE STROBEL, G., PASINETTI, L.E. 1975: ASTRON.ASTROPHYS. 43, 127 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: ANALYSIS: LTE(PEYTREMANN 1974), DIFF(EPS VIR), T+G(FE I/II IONIZATION, R-I, WEAK+STRONG MG LINES, CHECKED BY LINE PROFILES OF MG I B, NA I D, FE 5408+5434) REMARKS : OBSERVED COG ARE EXTENDED BY WEAK LINE DATA INTO THE LINEAR REGIME COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 6582 MU CAS G5VB (SUBDWARF) AR 01 04.9 DEC +54 41 MV = 5.17 FE/H = -- R ------------------------------------------------------------------------ ( 57) CATCHPOLE, A.M., PAGEL, B.E.J., POWELL, A.L.T. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 136, 403 ........................................................................ OBSERV. : PG, 4680-6770A, 6.8 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: 199, LLWW: CATCHPOLE ET AL. 1969: ROY.OBS.BULL. 154 ANALYSIS: COG, DIFF(SUN), T(R-I, FE I EXCITATION), PE(IONIZATION FE I/II, TI I/II) REMARKS : STRONG LINES (EQUIV.WIDTHS GREATER 160 MA) ARE NOT USED IN THE ANALYSIS COMMENTS: CLASS : DTGAA ------------------------------------------------------------------------ ( 44) COHEN, J.G. 1968: ASTROPHYS.J. 154, 179 ........................................................................ OBSERV. : PG, 4650-4900A, 5100-6250A, 4.5 A/MM INSTRUM.: MT.PALOMAR 200-INCH LINELIST: 250, DAOR ANALYSIS: LTE(STROM), T+G(IONIZATION, FE I EXCITATION), F-VALUES: DIFF(SUN) REMARKS : STRONG LINES (EQUIV.WIDTHS GREATER 160 MA) ARE NOT USED IN THE ANALYSIS COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3800-4700A, 9+13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(R-I, B-V, B-Y) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) REMARKS : SPECTRUM SYNTHESIS OF MOLECULAR BANDS COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (312) TOMKIN, J., LAMBERT, D.L., 1980: ASTROPHYS.J. 235, 925 ........................................................................ OBSERV. : PE, RETICON, 5130-5150A, 0.08A, S/N=100 INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE LINELIST: 4 MGH LINES, 4 FE I LINES ANALYSIS: LTE(GUSTAFSSON), T(R-I) REMARKS : DERIVE ABUNDANCES OF MG ISOTOPES FROM MGH BAND LINES COMMENTS: CLASS : (T)MA, L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 6755 BD +60 170 F8V (WEAK METALS) AR 01 06.5 DEC +61 17 MV = 7.73 FE/H = --- R ------------------------------------------------------------------------ ( 42) KOELBLOED, D. 1969: ASTROPHYS.J. 149, 299 ........................................................................ OBSERV. : PG, ??? , 9+14 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR, 300 ANALYSIS: COG, DIFF(SUN), T(COG) REMARKS : EXTREME HIGH VELOCITY STAR COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : DAA ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O KOELBLOED'S N ABUND. WAS BASED ON SINGLE, BLENDED CN LINE COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, R ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 6833 BD +53 236 G9III (EMISS H+K, WEAK METALS) AR 01 06.8 DEC +54 28 MV = 6.75 FE/H = --- R ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : PG, 4400-6800A, 9.7+12.4 A/MM, 0.3A INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(EPS VIR), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : COMMENTS: CLASS : DTGMAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : DATA FROM ( 41) CAYREL DE STROBEL 1966: ANN.AP. 29, 413 INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY REF.(41) DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 6860 BET AND M0III VAR (EMISS H+K) AR 01 06.9 DEC +35 21 MV = 2.06 FE/H = - R ------------------------------------------------------------------------ (247) HANNI, L., KIPPER, M. 1975: PUBL.TARTU ASTROFIZ. OBS. 43, 51 ........................................................................ OBSERV. : PG, 5050-6150A, 6 A/MM INSTRUM.: 100-INCH LINELIST: LLWW, 600: ANALYSIS: COG, T(???), F-VALUES WOLNIK ET AL.1970: AP.J. 162, 1037 (?) COMPARISON WITH THEOR. COG OF WRUBEL 1949: AP.J. 109, 66 REMARKS : COMMENTS: I CAN'T READ RUSSIAN WELL CLASS : TAA ------------------------------------------------------------------------ (A10) SMITH, V.V., LAMBERT, D.L. 1985: ASTROPHYS.J. 294, 326 ........................................................................ OBSERV. : PE, REGIONS BETWEEN 7330-7600 A, 0.2 A (RETICON) 1.6 + 2.2 MICRON (4500 CM**-1), 0.05 CM**-1 (FTS) INSTRUM.: MCDONALD 2.7M, COUDE, RETICON; KPNO 4M, FTS LINELIST: LW, 29 ATOMIC + 60 MOLECULAR LINES ANALYSIS: LTE(JOHNSON), DIFF(ALF TAU), T(V-K), G(ABS.MAG.+EVOL.TRACKS) F-VALUES: CF. LAMBERT ET AL. 1984: AP.J. 284, 223 REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 7424 BD -17 219 G0 AR 01 11.6 DEC -16 41 MV = 10.08 FE/H = - R? ------------------------------------------------------------------------ (346) PETERSON, R.C. 1981: ASTROPHYS.J.SUPPL. 45, 421 ........................................................................ OBSERV. : PG, IT, 5540-6750A, 3.1 A/MM INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: LLWW, 300: ANALYSIS: LTE(ATLAS, GUSTAFSSON), T(FE I EXCITATION), G(ASSUMED), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: CLASS : (D)TMA, R? ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (346) PETERSON 1980: ASTROPHYS.J.SUPPL. 45, 421 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 7583 RMC 45 A0IA0 AR 01 12.1 DEC -73 36 MV = 10.19 FE/H = 0 L ------------------------------------------------------------------------ (114) PRZYBYLSKI, A. 1972: MONTHLY NOTICES ROY.ASTRON.SOC. 159, 155 ........................................................................ OBSERV. : PG, 3700-4900A, 10 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: ANALYSIS: COG, DIFF(ALF CYG, HD 67456), T+PE(FE IONIZATION), F-VALUES FROM GARZ KOCK 1969: A+A 2, 274 AND BASCHEK ET AL.1970: A+A 4, 229 REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (207) WOLF, B. 1973: ASTRON.ASTROPHYS. 28, 335 ........................................................................ OBSERV. : PG, 3600-4900A, 12 A/MM, 5780-HALFA, 31 A/MM INSTRUM.: ESO 1.5M LINELIST: LLWW, 165 ANALYSIS: LTE, T+G(IONIZATION MG I/II, FE I/II; BALMER EQU.WIDTHS, BALMER JUMP), F-VALUES: FROM LISTED REFERENCES (...1969) REMARKS : COMMENTS: CLASS : TGMAA, L ======================================================================== HD 8512 TET CET K0III (EMISS H+K) AR 01 21.5 DEC -08 26 MV = 3.60 FE/H = 0 (R?) ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, (R?) ======================================================================== HD 8724 BD +16 149 G5 (WEAK METALS) AR 01 23.6 DEC +16 52 MV = 9.4 FE/H = --- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 8890 ALF UMI F7:IB-II VAR AR 01 48.8 DEC +89 02 MV = 2.02 FE/H = 0 (I) ------------------------------------------------------------------------ (136) KIPPER, T. 1969: PUBL.TARTU ASTROFIZ.OBS. 36, 227 ........................................................................ OBSERV. : DATA FROM PANNEKOEK 1950: PUBL.DOMINION AP.OBS. 8,1 INSTRUM.: LINELIST: ANALYSIS: COG(THEOR. COG FROM UNSOELD 1949: STELLAR ATMOSPHERES) REMARKS : DERIVES STELLAR VALUES FOR OSCILLATOR STRENGTHS COMMENTS: CLASS : TAA, (I) ======================================================================== HD 9826 UPS AND F9V AR 01 33.8 DEC +41 09 MV = 4.09 FE/H = 0 R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 98) SPITE, M., SPITE, F. 1973: ASTRON.ASTROPHYS. 23, 63 ........................................................................ OBSERV. : PG, 20A SECTIONS CENTERED AT 4450, 4550, 4580A, 2 A/MM INSTRUM.: OHP 1.9M, HI-RES. SPECTROGR., LALLEMAND EGC ALSO: OHP 1.5M, COUDE, HBETA LINE WINGS, 7 A/MM LINELIST: (MORE THAN 30): ANALYSIS: DIFF(SUN), LTE(PEYTREMANN) T(B2-V1,B-Y,G-I,BETA, HBETA WINGS) G(IONIZATION FE, TI, CR) REMARKS : MEASURE PRIMARILY THE FAINT LINES COMMENTS: FE/H IS GIVEN AS PRELIMINARY RESULT CLASS : (DTGMAA), R? ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 9927 51 AND K3III (EMISS H+K) AR 01 34.9 DEC +49 23 MV = 3.57 FE/H = 0 R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 9973 BD +60 296 F5IAB AR 01 35.7 DEC +60 50 MV = 6.88 FE/H = - (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 10307 HR 483 G1.5V AR 01 38.7 DEC +42 22 MV = 4.90 FE/H = 0 R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 74) SPINRAD, H., LUEBKE, W.R. 1970: ASTROPHYS.J. 160, 1141 ........................................................................ OBSERV. : PG, 5180-5880A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(COLOUR 5360-7400A) REMARKS : SUPER-METAL-RICH COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (128) BRANCH, D., BELL, R.A. 1971: MONTHLY NOT.ROY.ASTRON.SOC. 153, 57 ........................................................................ OBSERV. : PG, 5200-6240A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 262 ANALYSIS: THEOR.COG, T(COLOUR 5360-7400A) TEMP-TAU-RELATION: KRISHNA SWAMY 1967: AP.J. 150, 1161 FE F-VALUES: CORLISS(1968) REMARKS : COMMENTS: CLASS : T(M)AA, L ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 10476 7 PSC K1V AR 01 39.8 DEC +20 02 MV = 5.24 FE/H = 0 (R) ------------------------------------------------------------------------ (421) PERRIN, M.-N. 1983: ASTRON.ASTROPHYS. 128, 347 ........................................................................ OBSERV. : PG, 4800-5930A, 12.4 A/MM, 0.25 A, S/N=30 (OHP), RETICON, 6380-6630A, 0.25 A, S/N=200 (CFH) INSTRUM.: OHP 1.9M, CFH 3.6M, COUDE LINELIST: LLWW, 302 ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : HALFA LINE PROFILE IS ALSO REPRODUCED COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 10494 BD +61 316 F5IA AR 01 40.8 DEC +61 36 MV = 7.29 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 10700 TAU CET G8V AR 01 41.8 DEC -16 12 MV = 3.50 FE/H = - R ------------------------------------------------------------------------ ( 26) PAGEL, B.E.J. 1963: J.QUANT.SPECTROSC.RADIAT.TRANSFER 3, 139 ........................................................................ OBSERV. : PG, ??? INSTRUM.: MT.WILSON 100-INCH LINELIST: 156 ANALYSIS: COG, DIFF(SUN), EMPIRICAL COG FROM FE I LINES T(FE I EXCITATION) REMARKS : TESTS DIFFERENTIAL COG METHOD COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 5) PAGEL, B.E.J. 1964: ROY.OBS.BULL. 87 ........................................................................ OBSERV. : PG, 3700-4900A, 9+4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN), T(EMPIR. COG FROM FE I LINES) REMARKS : RGI COLOURS ARE USED AS A CHECK ON THE DERIVED TEMPERATURES COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (419) STEENBOCK, W. 1983: ASTRON.ASTROPHYS. 126, 325 ........................................................................ OBSERV. : PG, 4650-6050A, 3.3 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LW, 25: ANALYSIS: LTE(SCALED SOLAR T-TAU RELATION, ATLAS), DIFF(SUN), T(VRIJKL, MG I B LINE WINGS), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVE BA, FE, MG ABUNDANCES FROM SELECTED ISOLATED LINES COMMENTS: CLASS : DTGMA, R ======================================================================== HD 10780 HR 511 K0V (EMISS H+K) AR 01 44.1 DEC +63 36 MV = 5.63 FE/H = + (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 11007 HR 523 F8V AR 01 45.8 DEC +32 26 MV = 5.79 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 11092 BD +64 243 K5IAB-B AR 01 47.6 DEC +64 36 MV = 6.57 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 11377 BD -17 330 F5 AR 01 49.1 DEC -16 59 MV = 8.5 FE/H = 0 (R) ------------------------------------------------------------------------ (A30) LUCK, R.E., BOND, H.E. 1982: ASTROPHYS.J. 259, 792 ........................................................................ OBSERV. : PG, 3800-5000A, 9+10 A/MM; 50A SECTIONS IN 5100-7800A, 0.2A, S/N= 30..50 (RETICON) INSTRUM.: MT.WILSON 100-INCH, COUDE, RETICON, MT.PALOMAR 200-INCH LINELIST: 200 OR MORE ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 11397 BD -17 332 F8 AR 01 49.3 DEC -16 34 MV = 9.02 FE/H = 0 (R) ------------------------------------------------------------------------ (293) FOY, R. 1980: ASTRON.ASTROPHYS. 85, 287 ........................................................................ OBSERV. : PG, 5200?-6200?A, 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(T-TAU FROM PEYTREMANN 1974) ), T(G-I), G(FE I/II IONIZATION), T+G CHECKED BY: LINE PROFILES OF MG I B TRIPLET F-VALUES AS COMPILED BY FOY 1972: A+A, 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : SPECTRUM UNDEREXPOSED ABUND. OF ELEMENTS OTHER THAN FE, NA, BA WERE DERIVED FROM WEAK LINES DIFFERENTIALLY TO THE SUN COMMENTS: CLASS : (D)TGMAA, (R) ======================================================================== HD 11544 BD +55 437 G2IB AR 01 51.6 DEC +56 20 MV = 6.82 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 11909 IOT ARI K1VP (EMISS H+K) AR 01 54.6 DEC +17 34 MV = 5.10 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6700A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 12533 GAM1 AND K3IIB... (EMISS H+K) AR 02 00.8 DEC +42 05 MV = 2.26 FE/H = 0 R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 12929 ALF ARI K2III SB (EMISS H+K) AR 02 04.3 DEC +23 14 MV = 2.00 FE/H = - R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (294) BRANCH, D., BONNELL, J., TOMKIN, J. 1978: ASTROPHYS.J. 225, 902 ........................................................................ OBSERV. : PE, RETICON, 7700-7870A, 8680-8780A, 0.12 A INSTRUM.: MCDONALD 2.7M, ECHELLE LINELIST: LW, 18 ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T+G(TOMKIN ET AL.1975: AP.J. 199, 436) REMARKS : 30 LINES OF ELEMENTS OTHER THAN FE WERE ALSO MEASURED, BUT NOT FULLY ANALYZED COMMENTS: DERIVE FE ABUNDANCE ONLY CLASS : DMA, L ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 13555 ETA ARI F5V AR 02 10.0 DEC +20 59 MV = 5.20 FE/H = - (R) ------------------------------------------------------------------------ ( 98) SPITE, M., SPITE, F. 1973: ASTRON.ASTROPHYS. 23, 63 ........................................................................ OBSERV. : PG, 20A SECTIONS CENTERED AT 4450, 4550, 4580A, 2 A/MM INSTRUM.: OHP 1.9M, HI-RES. SPECTROGR., LALLEMAND EGC ALSO: OHP 1.5M, COUDE, HBETA LINE WINGS, 7 A/MM LINELIST: (MORE THAN 30): ANALYSIS: DIFF(UPS AND), LTE(PEYTREMANN) T(B2-V1,B-Y,G-I,BETA, HBETA WINGS) G(IONIZATION FE, TI, CR) REMARKS : MEASURE PRIMARILY THE FAINT LINES COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 13783 BD +64 312 G8V AR 02 13.0 DEC +64 44 MV = 8.29 FE/H = -- R? ------------------------------------------------------------------------ (346) PETERSON, R.C. 1981: ASTROPHYS.J.SUPPL. 45, 421 ........................................................................ OBSERV. : PG, IT, 5540-6750A, 3.1 A/MM INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: LLWW, 300: ANALYSIS: LTE(ATLAS, GUSTAFSSON), T(R-I, V-K, FE I EXCITATION), G(ASSUMED), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: CLASS : (D)TMA, R? ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (246) PETERSON 1980: ASTROPHYS.J.SUPPL. 45, 421 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 13974 DEL TRI G0V SB (EMISS H+K) AR 02 14.0 DEC +34 00 MV = 4.90 FE/H = - R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 5) PAGEL, B.E.J. 1964: ROY.OBS.BULL. 87 ........................................................................ OBSERV. : PG, 3700-4900A, 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN), T(EMPIR. COG FROM FE I LINES) REMARKS : RGI COLOURS ARE USED AS A CHECK ON THE DERIVED TEMPERATURES COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : DATA FROM ( 3) WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3300-4700A, 9+13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ======================================================================== HD 13979 CD -26 814 G0 (WEAK METALS) AR 02 13.1 DEC -26 09 MV = 8.9 FE/H = ---- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE, SINGER CAMERA LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 14662 HR 690 F7IB AR 02 20.4 DEC +55 08 MV = 6.28 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 14802 KAP FOR G0VA (EMISS H+K) AR 02 20.3 DEC -24 03 MV = 5.19 FE/H = 0 (L) ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), (L) ======================================================================== HD 14829 BD -11 452 A0 (HORIZONTAL BRANCH) AR 02 20.7 DEC -10 54 MV = 10.30 FE/H = -- R ------------------------------------------------------------------------ (405) KODAIRA, K., PHILIP, A.G.D. 1981: ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS, IAU COLLOQ. NO.68, A.G.D.PHILIP, D.S.HAYES EDS., L.DAVIS PRESS, SCHENECTADY, N.Y., P. 153 ........................................................................ OBSERV. : ??? 12.5 A/MM ?? INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: ANALYSIS: LTE(ATLAS), T+G(PHOTOMETRY, HDELTA PROFILE) REMARKS : GIVE FE/H ONLY COMMENTS: SUPERSEDED BY (A22) CLASS : TGMA ------------------------------------------------------------------------ (A22) KODAIRA, K., PHILIP, A.G.D. 1984: ASTROPHYS.J. 278, 208 ........................................................................ OBSERV. : PG, 3850-4300A, 12.5 A/MM INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), DIFF(HD 161817), T+G(B-V, C1, M1, HDELTA WING), F-VALUES: KURUCZ+PEYTREMANN 1975 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 16234 31 ARI F7V AR 02 33.9 DEC +12 14 MV = 5.68 FE/H = - (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 16417 LAM2 FOR G5IV AR 02 34.9 DEC -34 47 MV = 5.78 FE/H = 0 L ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 16895 TET PER F7V AR 02 40.8 DEC +49 01 MV = 4.10 FE/H = 0 R ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : CHAFFEE, F.H. 1970: ASTRON.ASTROPHYS. 4, 291 INSTRUM.: LINELIST: 11 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 16901 14 PER G0IB-II (EMISS H+K) AR 02 40.8 DEC +44 05 MV = 5.43 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 17081 PI CET B7V AR 02 41.7 DEC -14 04 MV = 4.25 FE/H = 0 R ------------------------------------------------------------------------ (374) WOLFF, S.C. 1970: ASTROPHYS.J.SUPPL. 15, 21 ........................................................................ OBSERV. : PG, 3860-4620A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LW, 22 SELECTED UNBLENDED LINES ANALYSIS: COG(WRUBEL 1949), T(SCAN 4000-8800A, LTE(MIHALAS 1966)), G(HGAMMA PROFILES, LTE(MIHALAS 1966)), F-VALUES: WARNER 1967, CORLISS, BOZMAN 1962 REMARKS : USES ONLY ONE OR TWO LINES PER ION, MOST OF WHICH LIE ON THE COG'S FLAT PORTION. COMMENTS: THIS STAR SERVES AS STANDARD FOR STUDY OF AP STARS CLASS : TG(M)A ------------------------------------------------------------------------ (331) HEACOX, W.D. 1979: ASTROPHYS.J.SUPPL. 41, 675 ........................................................................ OBSERV. : PG, 3100-4700A, 6.8 A/MM, 0.14 A, MN III (1285 A) INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LLWW, 80: ANALYSIS: LTE(KPA), T(C0,M0), G(HGAMMA, HDELTA) FE F-VALUES OF WARNER(1967), CORRECTED AFTER SMITH(1976) REMARKS : GIVES ABUNDANCES FOR XI = 0 AND 3 KM/S COMMENTS: CLASS : TGMAA ------------------------------------------------------------------------ (A25) ADELMAN, S.J. 1984: MONTHLY NOTICES ROY.ASTRON.SOC. 206, 637 ........................................................................ OBSERV. : PG, ??? , 2-8.9 A/MM INSTRUM.: MT.WILSON, MT.PALOMAR, LICK, KPNO LINELIST: 100:, LW: MICROFICHE MN 206/1 ANALYSIS: LTE(ATLAS), DIFF(SUN), T+G(SCAN 3300-7100A, HGAMMA PROFILE), F-VALUES: BLACKWELL, KORNBLITH+BRIDGES, AND OTHERS REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 17506 ETA PER K3IB... (EMISS H+K) AR 02 47.0 DEC +55 41 MV = 3.76 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 17925 HR 857 K2V (EMISS H+K) AR 02 50.1 DEC -12 58 MV = 6.00 FE/H = 0 (R) ------------------------------------------------------------------------ (421) PERRIN, M.-N. 1983: ASTRON.ASTROPHYS. 128, 347 ........................................................................ OBSERV. : PG, 4800-5930A, 12.4 A/MM, 0.25 A, S/N=30 INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 210 ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : HALFA LINE PROFILE IS ALSO REPRODUCED COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 17948 HR 860 F4V AR 02 52.0 DEC +61 19 MV = 5.60 FE/H = - (R) ------------------------------------------------------------------------ ( 98) SPITE, M., SPITE, F. 1973: ASTRON.ASTROPHYS. 23, 63 ........................................................................ OBSERV. : PG, 20A SECTIONS CENTERED AT 4450, 4550, 4580A, 2 A/MM INSTRUM.: OHP 1.9M, HI-RES. SPECTROGR., LALLEMAND EGC ALSO: OHP 1.5M, COUDE, HBETA LINE WINGS, 7 A/MM LINELIST: (MORE THAN 30): ANALYSIS: DIFF(UPS AND), LTE(PEYTREMANN) T(B2-V1,B-Y,G-I,BETA, HBETA WINGS) G(IONIZATION FE, TI, CR) REMARKS : MEASURE PRIMARILY THE FAINT LINES COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 17958 HR 861 K3IAB: AR 02 52.3 DEC +64 08 MV = 6.24 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 18391 BD +57 672 G0IA AR 02 56.0 DEC +57 28 MV = 6.90 FE/H = - (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 18474 HR 885 G5:III... AR 02 56.4 DEC +47 01 MV = 5.47 FE/H = 0 (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN, CH WEAK COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 19373 IOT PER G0V AR 03 05.4 DEC +49 25 MV = 4.05 FE/H = 0 R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : DATA FROM ( 3) WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : DATA FROM HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 INSTRUM.: LINELIST: 11 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ======================================================================== HD 19445 BD +25 495 G5VI (SUBDWARF) AR 03 05.5 DEC +26 09 MV = 8.05 FE/H = ---- R ------------------------------------------------------------------------ ( 11) CHAMBERLAIN, J.W., ALLER, L.H. 1951: ASTROPHYS.J. 114, 52 ........................................................................ OBSERV. : PG, 4064-4732A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 65: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66), LTE MODELS, F-VALUES: KING 1938+42, T+G(FE I/II IONIZATION, PROFILES OF HBETA, HGAMMA, HDELTA, AND CA I K LINES) REMARKS : DERIVE FE AND CA ABUNDANCES COMMENTS: CLASS : TG(M)A ------------------------------------------------------------------------ ( 38) ALLER, L.H., GREENSTEIN, J.L. 1960: ASTROPHYS.J.SUPPL. 5, 139 ........................................................................ OBSERV. : PG, 3650-4900A, 10 A/MM, 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE, MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 65: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66), T(SOLAR EXC.TEMP. ASSUMED), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : D(T)AA ------------------------------------------------------------------------ ( 58) COHEN, J.G., STROM, S.E. 1968: ASTROPHYS.J. 151, 623 ........................................................................ OBSERV. : DATA FROM ( 38) ALLER, GREENSTEIN 1960: AP.J.SUPPL. 5, 139 INSTRUM.: LINELIST: ANALYSIS: LTE(STROM ET AL.1966: AP.J. 146, 880), T(SCAN, HGAMMA, CF. STROM ET AL.1966: AP.J. 147, 1038), G(EVOLUT. TRACKS), T+G CHECKED BY FE EXCITATION+IONIZATION F-VALUES: CHECKED WITH SOLAR LINES REMARKS : COMMENTS: CLASS : (D)TGAA ------------------------------------------------------------------------ (244) GRABOWSKI, B. 1976: ACTA ASTRON. 26, 147 ........................................................................ OBSERV. : PG, 3600-4500A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG(WEIGHTING FUNCTIONS FROM LTE(CAYREL, JUGAKU) MODELS; COG SHAPE FROM SUN(COWLEY'S 1964: AP.J. 140, 713), UNSOELD 1968: STERNATMOSPHAEREN), DIFF(HD 140283, SUN), T(FE I EXCITATION; TI I/II IONIZATION, NE FROM BALMER LINES VIA INGLIS-TELLER FORMULA; HGAMMA PROFILE), F-VALUES: VARIOUS WORKS(1964-1975) AS LISTED REMARKS : COMMENTS: CLASS : DTMAA ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 120: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: CLASS : DTGMA, L ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM ( 38) ALLER, GREENSTEIN 1960: AP.J.SUPPL. 5, 139 INSTRUM.: LINELIST: USE LINES LONGWARD OF 4300 A ONLY ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(R-I), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-4620A, 1.48 A/MM, 0.18 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 120:, LLWW: PETERSON 1978: ASTROPHYS.J. 222, 181 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL, CA, TI ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA, R ------------------------------------------------------------------------ (A13) MAGAIN, P. 1985: ASTRON.ASTROPHYS. 132, 208 ........................................................................ OBSERV. : PG, 4000-4900A, 12.4 A/MM, 0.25 A, 9 COADDED SPECTRA, S/N= 100..200 INSTRUM.: OHP 1.5M, COUDE LINELIST: LW, 28 ANALYSIS: LTE(GUSTAFSON, EMPIRICAL T(TAU) RELATION FROM SCAN 4000..8000A, HGAMMA, HDELTA PROFILES)), T(R-I, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: LABORATORY(BLACKWELL 1982) REMARKS : USES ONLY LINES WITH EQUIV.WIDTHS 10..100 MA COMMENTS: EMPIRICAL TEMPERATURE(TAU) RELATION STEEPER THAN FROM GUSTAFSSON MODEL IN LAYERS DEEPER THAN TAU= 1 SUPERSEDED BY (A12) CLASS : TGMA ------------------------------------------------------------------------ (A12) MAGAIN, P. 1985: ASTRON.ASTROPHYS. 146, 95 ........................................................................ OBSERV. : DATA FROM (A13) MAGAIN 1985: A+A 132, 208 PG, 3500-4900A, 12.4 A/MM, 9 SPECTRA COADDED INSTRUM.: OHP 1.5M, COUDE LINELIST: LLWW, 160: ANALYSIS: LTE(EMPIRICAL T(TAU) FROM SCAN 4000-12000A), T(SCAN 4000-12000A, UV SHORTER THAN 3080A, V-K), G(FE I/II, TI I/II IONIZATION; STRONG LINES OF FE I, CA I; PROFILES OF CA II K, BALMER LINES; BJ), F-VALUES: LABORATORY(BLACKWELL 1982) REMARKS : EXTENSION OF (A13) COMMENTS: CLASS : TGMAA, R ======================================================================== HD 19476 KAP PER K0III (EMISS H+K) AR 03 06.1 DEC +44 40 MV = 3.80 FE/H = 0 R ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: OHP LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 20038 SAO 233021 F7IIIW... (WEAK METALS) AR 03 09.3 DEC -59 01 MV = 8.91 FE/H = --- (R) ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 20439 HYADES 2 G0 AR 03 14.9 DEC +07 30 MV = 7.76 FE/H = 0 (R) ------------------------------------------------------------------------ (323) BRANCH, D., LAMBERT, D.L., TOMKIN, J. 1980: ASTROPHYS.J. 241, L87 ........................................................................ OBSERV. : 100A WIDE REGIONS AT 6578, 6752A, 0.2 A, S/N= 300 INSTRUM.: MCDONALD 2.7M, COUDE, RETICON LINELIST: LW, 21 FE I LINES ANALYSIS: LTE(T-TAU SCALED FROM SUN(HOLWEGER, MUELLER 1974)), DIFF(SUN), T(HALFA PROFILE, LTE(ATLAS)), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTAA, (R) ======================================================================== HD 20630 KAP CET G5V VAR (EMISS H+K) AR 03 16.7 DEC +03 11 MV = 4.83 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 20766 ZET1 RET G2.5V AR 03 16.7 DEC -62 46 MV = 5.54 FE/H = 0 L ------------------------------------------------------------------------ ( 45) DANZIGER, I.J. 1966: ASTROPHYS.J. 143, 527 ........................................................................ OBSERV. : PG, 4000-4900A, 6.7 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 142 ANALYSIS: COG(SOLAR COG FROM ALLER 1953: ASTROPHYSICS, RONALD PRESS), DIFF(SUN), T(UVBGRI, EXCITATION), PE(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 20794 82 ERI G8V (EMISS H+K) AR 03 17.9 DEC -43 16 MV = 4.27 FE/H = - R ------------------------------------------------------------------------ ( 63) HEARNSHAW, J.B. 1973: ASTRON.ASTROPHYS. 29, 165 ........................................................................ OBSERV. : PG, 4300-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 80: ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTMA, R ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ------------------------------------------------------------------------ (419) STEENBOCK, W. 1983: ASTRON.ASTROPHYS. 126, 325 ........................................................................ OBSERV. : PG, 3500-6050A, 3.3 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LW, 25: ANALYSIS: LTE(SCALED SOLAR T-TAU RELATION, ATLAS), DIFF(SUN), T(VRI, MG I B LINE WINGS), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVE BA, FE, MG ABUNDANCES FROM SELECTED ISOLATED LINES COMMENTS: CLASS : DTGMA, R ======================================================================== HD 20807 ZET2 RET G1V AR 03 17.1 DEC -62 42 MV = 5.24 FE/H = - R ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 20902 ALF PER F5IAB: AR 03 20.7 DEC +49 41 MV = 1.79 FE/H = 0 I ------------------------------------------------------------------------ (156) GREENSTEIN, J.L. 1948: ASTROPHYS.J. 107, 151 ........................................................................ OBSERV. : PG, 4010-4830A, 2.8 A/MM INSTRUM.: MCDONALD, COUDE LINELIST: LLWW, 350 ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION) REMARKS : COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ (167) WRIGHT, K.O. 1951: PUBL.DOM.ASTROPHYS.OBS.VICTORIA 8, 1 ........................................................................ OBSERV. : PG, 3700-6750A, 4.8...20.8 A/MM INSTRUM.: DAO 72-INCH, CASSEGRAIN LINELIST: LLWW, 800 ANALYSIS: COG, DIFF(SUN), THEO.COG MENZEL, UNSOELD 1936: AP.J. 84, 474 T(FE I, TI I EXCITATION) REMARKS : COMMENTS: OBSERVATIONS WERE DONE BETWEEN 1937-1945 CLASS : DTAA, I ======================================================================== HD 21389 HR 1040 A0IAB: AR 03 25.9 DEC +58 42 MV = 4.54 FE/H = ? (L) ------------------------------------------------------------------------ (172) AYDIN, C. 1972: ASTRON.ASTROPHYS. 19, 369 ........................................................................ OBSERV. : PG, 3710-4860A, 12.4 A/MM INSTRUM.: OHP 1.5M, 1.9M, COUDE LINELIST: 280:, LLWW: AYDIN 1972: ASTRON.ASTROPHYS.SUPPL. 7, 331 ANALYSIS: COG, DIFF(ALF CYG), T+G(HBETA, HGAMMA, BALMER DISC.), PE(FE I/II IONIZATION, INGLIS-TELLER) F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVES FE, TI, CR ABUNDANCES ONLY COMMENTS: CLASS : DTGA, (L) ======================================================================== HD 21581 BD -00 552 G0 AR 03 26.3 DEC -00 35 MV = 8.3 FE/H = --- R? ------------------------------------------------------------------------ (346) PETERSON, R.C. 1981: ASTROPHYS.J.SUPPL. 45, 421 ........................................................................ OBSERV. : PG, IT, 5540-6750A, 3.1 A/MM INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: LLWW, 300: ANALYSIS: LTE(ATLAS, GUSTAFSSON), T(R-I), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: CLASS : (D)TMA, R? ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (246) PETERSON 1980: ASTROPHYS.J.SUPPL. 45, 421 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON, ATLAS), T(R-I), G(FE, TI IONIZATION), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 22049 EPS ERI K2V (EMISS H+K) AR 03 30.6 DEC -09 38 MV = 3.73 FE/H = 0 R ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (419) STEENBOCK, W. 1983: ASTRON.ASTROPHYS. 126, 325 ........................................................................ OBSERV. : PG, 3500-6050A, 3.3 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LW, 25: ANALYSIS: LTE(SCALED SOLAR T-TAU RELATION, ATLAS), DIFF(SUN), T(VRIJKL, MG I B LINE WINGS), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVE BA, FE, MG ABUNDANCES FROM SELECTED ISOLATED LINES COMMENTS: CLASS : DTGMA, R ======================================================================== HD 22484 10 TAU F9IV-V AR 03 34.3 DEC +00 15 MV = 4.28 FE/H = 0 R ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA PROFILE), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 22879 BD -03 592 F9V (EMISS H+K) AR 03 37.8 DEC -03 22 MV = 6.74 FE/H = -- (L) ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 23194 PLEIADES 232 A5V AR 03 41.0 DEC +24 24 MV = 8.05 FE/H = 0 (L) ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(HGAMMA, FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, (L) ======================================================================== HD 23249 DEL ERI K0IV AR 03 40.8 DEC -09 54 MV = 3.53 FE/H = 0 R ------------------------------------------------------------------------ ( 13) HAZELHURST, J. 1963: OBSERVATORY 83, 128 ........................................................................ OBSERV. : PG, 5700-6500A, 6.5 A/MM; 4400-4600A, 4.5 A/MM; 4100-4400A, 2 A/MM INSTRUM.: MT.WILSON??? LINELIST: ANALYSIS: COG(SUN, ETA CEP), T(SCAN 4500-5800A), PE(TI I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : FROM 6.5 A/MM DATA DERIVES V, TI, NI, FE ABUNDANCES, RESULTS FROM ANALYSIS OF 2 A/MM DATA ON 18 OTHER ELEMENTS ARE GIVEN QUALITALTIVELY COMMENTS: SHORT COMMUNICATION CLASS : DTA ------------------------------------------------------------------------ ( 22) PAGEL, B.E.J. 1963: OBSERVATORY 83, 133 ........................................................................ OBSERV. : PG, ??? , 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(R-I) REMARKS : COMMENTS: PROBABLY SUPERSEDED BY ( 5) PAGEL (1964) CLASS : DTAA ------------------------------------------------------------------------ ( 5) PAGEL, B.E.J. 1964: ROY.OBS.BULL. 87 ........................................................................ OBSERV. : PG, 3900-4850A, 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN), T(EMPIR. COG FROM FE I LINES) REMARKS : RGI COLOURS ARE USED AS A CHECK ON THE DERIVED TEMPERATURES COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(R-I) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : PG, 4500-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, EGC LINELIST: LLWW, 150: ANALYSIS: DIFF(SUN), LTE(PEYTREMANN 1974) T(R-I, I-K) G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUND. ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : DATA FROM (245) HEARNSHAW 1976: A+A 51, 71 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION), F-VALUES: FOY (1972) REMARKS : REANALYSIS COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 23269 PLEIADES 405 F9V AR 03 41.7 DEC +24 41 MV = 9.82 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4700A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 14 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 23386 PLEIADES 739 G0V AR 03 42.7 DEC +24 46 MV = 9.56 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4700A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 14 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 23387 PLEIADES 717 A1V AR 03 42.6 DEC +24 11 MV = 7.16 FE/H = - (L) ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(B-V, FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, (L) ======================================================================== HD 23439A ??? K1VB AR 03 43.6 DEC +41 18 MV = ? FE/H = --- L? ------------------------------------------------------------------------ (346) PETERSON, R.C. 1981: ASTROPHYS.J.SUPPL. 45, 421 ........................................................................ OBSERV. : PG, IT, 5540-6750A, 3.1 A/MM INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: LLWW, 300: ANALYSIS: LTE(ATLAS, GUSTAFSSON), T(R-I), G(ASSUMED), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: CLASS : (D)TMA, L? ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (346) PETERSON 1980: ASTROPHYS.J.SUPPL. 45, 421 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 23439B BD +41 750A K1V AR 03 43.6 DEC +41 18 MV = 8.74 FE/H = --- (L) ------------------------------------------------------------------------ (346) PETERSON, R.C. 1981: ASTROPHYS.J.SUPPL. 45, 421 ........................................................................ OBSERV. : PG, IT, 5540-6750A, 3.1 A/MM INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: LLWW, 300: ANALYSIS: LTE(ATLAS, GUSTAFSSON), T(R-I), G(ASSUMED), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: CLASS : (D)TMA, L? ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (346) PETERSON 1980: ASTROPHYS.J.SUPPL. 45, 421 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 23464 PLEIADES 948 G0V AR 03 43.3 DEC +22 58 MV = 8.66 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4700A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 14 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 23607 PLEIADES 1362 A7V AR 03 44.3 DEC +23 59 MV = 8.26 FE/H = - (L) ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(HGAMMA, FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, (L) ======================================================================== HD 23631 PLEIADES 1397 A2V AR 03 44.4 DEC +23 46 MV = 7.26 FE/H = 0 (L) ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(B-V, FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, (L) ======================================================================== HD 23713 PLEIADES 1726 F6V AR 03 45.1 DEC +23 59 MV = 9.25 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4700A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 14 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 23732 PLEIADES 1766 F4V AR 03 45.3 DEC +25 04 MV = 9.12 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4700A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 14 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 23841 BD +09 494 K1III AR 03 45.8 DEC +09 30 MV = 6.69 FE/H = -- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 23924 PLEIADES 2415 A7V AR 03 46.7 DEC +23 11 MV = 8.10 FE/H = - (L) ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(HGAMMA, FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, (L) ======================================================================== HD 23964 PLEIADES 2507 A0V... AR 03 47.0 DEC +23 42 MV = 6.74 FE/H = 0 (L) ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(B-V, FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, (L) ======================================================================== HD 24368 PLEIADES 5030 A2V AR 03 50.6 DEC +25 32 MV = 6.33 FE/H = 0 (L) ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(SPEC.TYPE, FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, (L) ======================================================================== HD 25329 BD +34 796 K1V... (SUBDWARF) AR 03 59.9 DEC +35 09 MV = 8.50 FE/H = --- R ------------------------------------------------------------------------ ( 46) PAGEL, B.E.J, POWELL, A.L.T. 1966: ROY.OBS.BULL. 124 ........................................................................ OBSERV. : PG, 4006-4861A, 10 A/MM (MT.WILSON) 4703-5233A, 5296-6265A, 10 A/MM (MT.PALOMAR) INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 175 ANALYSIS: COG, DIFF(SUN), T(EMPIR. COG FROM FE I LINES, GRI), ALSO USE LTE(CAYREL, JUGAKU) REMARKS : COMMENTS: CLASS : DT(M)AA, L ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : DATA FROM ( 46) PAGEL, POWELL 1966: ROY.OBS.BULL. 124 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTMA, R ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : DATA FROM ( 46) PAGEL, POWELL 1966: ROY.OBS.BULL. 124 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION), F-VALUES: FOY (1972) REMARKS : HEARNSHAW 1976: A+A 51, 71 MAY HAVE USED BLENDED FE II LINE COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (346) PETERSON, R.C. 1981: ASTROPHYS.J.SUPPL. 45, 421 ........................................................................ OBSERV. : PG, IT, 5540-6750A, 3.1 A/MM INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: LLWW, 300: ANALYSIS: LTE(ATLAS, GUSTAFSSON), T(R-I, V-K, SCAN ???, FE I EXCITATION), G(ASSUMED), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: CLASS : (D)TMA, R? ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (346) PETERSON 1980: ASTROPHYS.J.SUPPL. 45, 421 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 25532 BD +22 626 F6IV-V (WEAK METALS) AR 04 01.2 DEC +23 16 MV = 8.18 FE/H = --- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 25825 HYADES 10 G0 AR 04 03.4 DEC +15 34 MV = 7.85 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 26297 BD -16 791 G1V AR 04 06.8 DEC -16 01 MV = 7.6 FE/H = --- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE, SINGER CAMERA LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 26462 45 TAU F4V AR 04 08.7 DEC +05 24 MV = 5.70 FE/H = 0 R ------------------------------------------------------------------------ (223) CONTI, P.S., WALLERSTEIN, G., WING, R.F. 1965: ASTROPHYS.J. 142, 999 ........................................................................ OBSERV. : PG, 3850-6800A, 10.5+16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 400: ANALYSIS: COG(THEOR. COG FROM LTE(MIHALAS 1965) MODELS), DIFF(HD 28344), T(B-V), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTMAA, L ------------------------------------------------------------------------ (291) TOMKIN, J., LAMBERT, D.L., 1978: ASTROPHYS.J. 223, 937 ........................................................................ OBSERV. : PE, 100A SECTIONS IN THE RANGE 6500-9300A, 0.2A, S/N= 500 INSTRUM.: MCDONALD 2.7M, COUDE, SI PHOTODIODE ARRAY LINELIST: LW, 56: ANALYSIS: LTE(ATLAS), T+G(B-Y, C1; BETA), F-VALUES: DIFF(SUN, HOLWEGER-MUELLER MODEL), THEORETICAL REMARKS : DERIVE C, N, O, FE ABUNDANCES COMMENTS: CLASS : (D)TA, R ======================================================================== HD 26630 MU PER G0IB (EMISS H+K) AR 04 11.2 DEC +48 17 MV = 4.10 FE/H = 0 R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 5000-6650A, 6.5 A/MM INSTRUM.: MT.WILSON 100-INCH LINELIST: 800:, LLWW: VAN PARADIJS 1973: A+A SUPPL. 11, 25 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (352) FOY, R. 1981: ASTRON.ASTROPHYS. 103, 135 ........................................................................ OBSERV. : DATA FROM (264) LUCK 1977: AP.J. 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T(LUCK), G(IONIZATION FE, TI, CR), F-VALUES: FOY 1972: A+A 18, 26 REMARKS : REANALYIS, GIVE RESULTS ON FE/H ONLY COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 26736 HYADES 15 G5 AR 04 11.5 DEC +23 27 MV = 8.09 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 26756 HYADES 17 G5 AR 04 11.6 DEC +14 30 MV = 8.46 FE/H = 0 L ------------------------------------------------------------------------ (223) CONTI, P.S., WALLERSTEIN, G., WING, R.F. 1965: ASTROPHYS.J. 142, 999 ........................................................................ OBSERV. : PG, 3850-6800A, 10.5+16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 400: ANALYSIS: COG(THEOR. COG FROM LTE(MIHALAS 1965) MODELS), DIFF(HD 28344), T(B-V), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTMAA ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, L ======================================================================== HD 26767 HYADES 18 G0 AR 04 11.7 DEC +12 19 MV = 8.06 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 26965 OMI2 ERI K1V (EMISS H+K) AR 04 13.0 DEC -07 44 MV = 4.41 FE/H = - R ------------------------------------------------------------------------ ( 5) PAGEL, B.E.J. 1964: ROY.OBS.BULL. 87 ........................................................................ OBSERV. : PG, 3700-4900A, 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN), T(EMPIR. COG FROM FE I LINES) REMARKS : RGI COLOURS ARE USED AS A CHECK ON THE DERIVED TEMPERATURES COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (419) STEENBOCK, W. 1983: ASTRON.ASTROPHYS. 126, 325 ........................................................................ OBSERV. : PG, 4650-6050A, 3.3 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LW, 25: ANALYSIS: LTE(SCALED SOLAR T-TAU RELATION, ATLAS), DIFF(SUN), T(VRIJKL, MG I B LINE WINGS), N, ATLAS), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVE BA, FE, MG ABUNDANCES FROM SELECTED ISOLATED LINES COMMENTS: CLASS : DTGMA, R ======================================================================== HD 27371 GAM TAU K0III (EMISS H+K) AR 04 17.0 DEC +15 31 MV = 3.65 FE/H = 0 R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ ( 6) HELFER, H.L., WALLERSTEIN, G. 1964: ASTROPHYS.J.SUPPL. 9, 81 ........................................................................ OBSERV. : PG, 5100-6700A, 6+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 350: ANALYSIS: COG(AVERAGED EMPIRICAL COG FROM FE I), DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 47) GRIFFIN, R. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 413, 381 ........................................................................ OBSERV. : PG, 5190-6260A, 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 600: ANALYSIS: COG(EMPIR. FROM ALF BOO), DIFF(ALF BOO), T(FE I , TI I EXCITATION; RIJKL), PE( FI, FE IONIZATION), F-VALUES: DIFF(ALF BOO) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN ??? INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY ??? DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : DATA FROM ( 6) HELFER, WALLERSTEIN 1964: AP.J.SUPPL. 9, 81 INSTRUM.: LINELIST: 85 FE I, 25 FE II LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL 1963: AP.J. 137, 431 INSTRUM.: LINELIST: ANALYSIS: DIFF(SUN), LTE(ATLAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.4 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 7 A/MM INSTRUM.: OHP LINELIST: TO BE PUBLISHED ANALYSIS: COG(LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, R ------------------------------------------------------------------------ (380) KOMAROV, N.S., SHCHERBAK, A.N. 1980: SOVIET ASTRON. 24, 323 ........................................................................ OBSERV. : GRIFFIN 1969: MNRAS 143, 381 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(ALF BOO), T(FE I EXCITATION), PE(FE I/II IONZATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 27383 HYADES 29 F9V AR 04 17.0 DEC +16 24 MV = 6.86 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 27561 HYADES 37 F5V AR 04 18.8 DEC +14 18 MV = 6.60 FE/H = 0 R ------------------------------------------------------------------------ (223) CONTI, P.S., WALLERSTEIN, G., WING, R.F. 1965: ASTROPHYS.J. 142, 999 ........................................................................ OBSERV. : PG, 3850-6800A, 10.5+16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 400: ANALYSIS: COG(THEOR. COG FROM LTE(MIHALAS 1965) MODELS), DIFF(HD 28344), T(B-V), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTMAA, L ------------------------------------------------------------------------ (291) TOMKIN, J., LAMBERT, D.L., 1978: ASTROPHYS.J. 223, 937 ........................................................................ OBSERV. : PE, 100A SECTIONS IN THE RANGE 6500-9300A, 0.2A, S/N= 500 INSTRUM.: MCDONALD 2.7M, COUDE, SI PHOTODIODE ARRAY LINELIST: LW, 56: ANALYSIS: LTE(ATLAS), T+G(B-Y, C1; BETA), F-VALUES: DIFF(SUN, HOLWEGER-MUELLER MODEL), THEORETICAL REMARKS : DERIVE C, N, O, FE ABUNDANCES COMMENTS: CLASS : (D)TA, R ======================================================================== HD 27685 HYADES 39 G4V AR 04 19.9 DEC +16 40 MV = 7.86 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 27697 DEL1 TAU K0III (EMISS H+K) AR 04 20.0 DEC +17 26 MV = 3.76 FE/H = 0 R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ ( 6) HELFER, H.L., WALLERSTEIN, G. 1964: ASTROPHYS.J.SUPPL. 9, 81 ........................................................................ OBSERV. : PG, 5100-6700A, 6+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 350: ANALYSIS: COG(AVERAGED EMPIRICAL COG FROM FE I), DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN ??? INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY ??? DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : DATA FROM ( 6) HELFER, WALLERSTEIN 1964: AP.J.SUPPL. 9, 81 INSTRUM.: LINELIST: 85 FE I, 25 FE II LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL 1963: AP.J. 137, 431 INSTRUM.: LINELIST: ANALYSIS: DIFF(SUN), LTE(ATLAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (294) BRANCH, D., BONNELL, J., TOMKIN, J. 1978: ASTROPHYS.J. 225, 902 ........................................................................ OBSERV. : PE, RETICON, 7700-7870A, 8680-8780A, 0.12 A INSTRUM.: MCDONALD 2.7M, ECHELLE LINELIST: LW, 18 ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T+G(LAMBERT, RIES 1977: AP.J. 217, 508) REMARKS : 30 LINES OF ELEMENTS OTHER THAN FE WERE ALSO MEASURED, BUT NOT FULLY ANALYZED COMMENTS: DERIVE FE ABUNDANCE ONLY CLASS : DMA, R ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: OHP LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, L ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 27808 HYADES 48 F8V AR 04 21.3 DEC +21 37 MV = 7.14 FE/H = 0 (L) ------------------------------------------------------------------------ (223) CONTI, P.S., WALLERSTEIN, G., WING, R.F. 1965: ASTROPHYS.J. 142, 999 ........................................................................ OBSERV. : PG, 3850-6800A, 10.5+16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 400: ANALYSIS: COG(THEOR. COG FROM LTE(MIHALAS 1965) MODELS), DIFF(HD 28344), T(B-V), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTMAA, (L) ======================================================================== HD 27819 DEL2 TAU A7V AR 04 21.2 DEC +17 20 MV = 4.80 FE/H = 0 I ------------------------------------------------------------------------ (223) CONTI, P.S., WALLERSTEIN, G., WING, R.F. 1965: ASTROPHYS.J. 142, 999 ........................................................................ OBSERV. : PG, 3850-8662A, 10.5+16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 400: ANALYSIS: COG(THEOR. COG FROM LTE(MIHALAS 1965) MODELS), DIFF(HD 28344), T(B-V), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTMAA, I ------------------------------------------------------------------------ ( 65) STROM, S.E., STROM, K.M. 1966: ASTRON.J. 71, 181 ........................................................................ OBSERV. : DATA FROM WRIGHT ET AL.1964: PUBL.DOMINION AP.OBS. 12, 173 INSTRUM.: LINELIST: ANALYSIS: LTE(STROM ET AL.1965: ASTRON.J. 70, 148) REMARKS : COMMENTS: SHORT COMMUNICATION CLASS : MAA ======================================================================== HD 27836 HYADES 50 G1V AR 04 21.4 DEC +14 39 MV = 7.62 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 27859 HYADES 52 G2V AR 04 21.6 DEC +16 46 MV = 7.80 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 27989 HYADES 58 G5V AR 04 22.9 DEC +18 45 MV = 7.53 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 28068 HYADES 63 G1V (EMISS H+K) AR 04 23.5 DEC +16 44 MV = 8.06 FE/H = 0 R? ------------------------------------------------------------------------ ( 28) WALLERSTEIN, G., HELFER, H.L. 1959: ASTROPHYS.J. 129, 347 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTGAA ------------------------------------------------------------------------ ( 29) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1960: ASTROPHYS.J. 132, 553 ........................................................................ OBSERV. : DATA FROM ( 28) WALLERSTEIN ET AL.1959: AP.J. 129, 347 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : REANALYSIS, BECAUSE A SMALL TERM IN SAHA'S EQUATION HAD BEEN NEGLECTED IN THE PREVIOUS ANALYSIS COMMENTS: CLASS : DTGAA, L ------------------------------------------------------------------------ ( 30) PARKER, R., GREENSTEIN, J.L., HELFER, H.L., WALLERSTEIN, G. 1961: ASTROPHYS.J. 133, 101 ........................................................................ OBSERV. : PG, ??? , 7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION) REMARKS : RE-ANALYSIS WITH NEW DATA CONFIRMS RESULTS FROM ( 28) WALLERSTEIN, HELFER 1959: AP.J. 129, 347 COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : DATA FROM ( 28) WALLERSTEIN, HELFER 1959: AP.J. 129, 247 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN ??? INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY ??? DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA ------------------------------------------------------------------------ (295) FOY, R. 1976: IAU SYMPOS. 72, B.HAUCK P.C.KEENAN EDS., 209 ........................................................................ OBSERV. : PG, ??? , 6 A/MM INSTRUM.: OHP, ECHELLE, LALLEMAND EGC LINELIST: ANALYSIS: COG(THEOR. COG FROM LTE(PEYTREMANN) MODELS), T(COLOURS, IONIZATION), DIFF(SUN)? REMARKS : COMMENTS: SHORT COMMUNICATION, GIVES FE/H ONLY CLASS : TMA, R? ======================================================================== HD 28099 HYADES 64 G2V AR 04 23.8 DEC +16 38 MV = 8.12 FE/H = 0 R ------------------------------------------------------------------------ ( 30) PARKER, R., GREENSTEIN, J.L., HELFER, H.L., WALLERSTEIN, G. 1961: ASTROPHYS.J. 133, 101 ........................................................................ OBSERV. : PG, 5150-6270A?, 14 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, ???? ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (323) BRANCH, D., LAMBERT, D.L., TOMKIN, J. 1980: ASTROPHYS.J. 241, L87 ........................................................................ OBSERV. : 100A WIDE REGIONS AT 6578, 6752A, 0.2 A, S/N= 300 INSTRUM.: MCDONALD 2.7M, COUDE, RETICON LINELIST: LW, 21 FE I LINES ANALYSIS: LTE(T-TAU SCALED FROM SUN(HOLWEGER, MUELLER 1974)), DIFF(SUN), T(HALFA PROFILE, LTE(ATLAS)), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTAA, R ======================================================================== HD 28305 EPS TAU G9.5III (EMISS H+K) AR 04 25.7 DEC +19 04 MV = 3.50 FE/H = 0 R ------------------------------------------------------------------------ ( 6) HELFER, H.L., WALLERSTEIN, G. 1964: ASTROPHYS.J.SUPPL. 9, 81 ........................................................................ OBSERV. : PG, 5100-6700A, 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 350: ANALYSIS: COG(AVERAGED EMPIRICAL COG FROM FE I), DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN ??? INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY ??? DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : DATA FROM ( 6) HELFER, WALLERSTEIN 1964: AP.J.SUPPL. 9, 81 INSTRUM.: LINELIST: 85 FE I, 25 FE II LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL 1963: AP.J. 137, 431 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS; CARBON, GINGERICH), DIFF(SUN), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.4+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: ESO LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, L ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 28307 TET1 TAU K0IIIB (EMISS H+K) AR 04 25.7 DEC +15 51 MV = 3.80 FE/H = 0 R ------------------------------------------------------------------------ ( 6) HELFER, H.L., WALLERSTEIN, G. 1964: ASTROPHYS.J.SUPPL. 9, 81 ........................................................................ OBSERV. : PG, 5100-6700A, 6+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 350: ANALYSIS: COG(AVERAGED EMPIRICAL COG FROM FE I), DIFF(MEAN OF GAM TAU, DEL TAU, EPS TAU), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 47) GRIFFIN, R. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 413, 381 ........................................................................ OBSERV. : PG, 5190-6260A, 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 600: ANALYSIS: COG(EMPIR. FROM ALF BOO), DIFF(ALF BOO), T(FE I , TI I EXCITATION; RIJKL), PE( FI, FE IONIZATION), F-VALUES: DIFF(ALF BOO) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : DATA FROM ( 41) CAYREL DE STROBEL 1966: ANN.AP. 29, 413 INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY REF.(41) DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.4 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : GRIFFIN, R. 1969: MNRAS 143, 381 INSTRUM.: LINELIST: 23 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, R ------------------------------------------------------------------------ (380) KOMAROV, N.S., SHCHERBAK, A.N. 1980: SOVIET ASTRON. 24, 323 ........................................................................ OBSERV. : DATA FROM GRIFFIN 1969: MNRAS 143, 381 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(ALF BOO), T(FE I EXCITATION), PE(FE I/II IONZATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 28344 HYADES 73 G2V AR 04 25.9 DEC +17 11 MV = 7.85 FE/H = 0 R ------------------------------------------------------------------------ ( 28) WALLERSTEIN, G., HELFER, H.L. 1959: ASTROPHYS.J. 129, 347 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTGAA ------------------------------------------------------------------------ ( 29) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1960: ASTROPHYS.J. 132, 553 ........................................................................ OBSERV. : DATA FROM ( 28) WALLERSTEIN ET AL.1959: AP.J. 129, 347 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : REANALYSIS, BECAUSE A SMALL TERM IN SAHA'S EQUATION HAD BEEN NEGLECTED IN THE PREVIOUS ANALYSIS COMMENTS: CLASS : DTGAA, L ------------------------------------------------------------------------ ( 30) PARKER, R., GREENSTEIN, J.L., HELFER, H.L., WALLERSTEIN, G. 1961: ASTROPHYS.J. 133, 101 ........................................................................ OBSERV. : PG, ??? , 14 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION) REMARKS : RE-ANALYSIS WITH NEW DATA CONFIRMS RESULTS FROM ( 28) WALLERSTEIN, HELFER 1959: AP.J. 129, 347 COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : DATA FROM ( 28) WALLERSTEIN, HELFER 1959: AP.J. 129, 347 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : DATA FROM ( 3) WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA, L ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN ??? INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY ??? DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ (295) FOY, R. 1976: IAU SYMPOS. 72, B.HAUCK P.C.KEENAN EDS., 209 ........................................................................ OBSERV. : PG, ??? , 6 A/MM INSTRUM.: OHP, ECHELLE, LALLEMAND EGC LINELIST: ANALYSIS: COG(THEOR. COG FROM LTE(PEYTREMANN) MODELS), T(COLOURS, IONIZATION), DIFF(SUN)? REMARKS : COMMENTS: SHORT COMMUNICATION, GIVES FE/H ONLY CLASS : TMA, R ======================================================================== HD 28483 HYADES 81 F5 AR 04 27.4 DEC +19 44 MV = 7.10 FE/H = 0 (L) ------------------------------------------------------------------------ (223) CONTI, P.S., WALLERSTEIN, G., WING, R.F. 1965: ASTROPHYS.J. 142, 999 ........................................................................ OBSERV. : PG, 3850-6800A, 10.5+16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 400: ANALYSIS: COG(THEOR. COG FROM LTE(MIHALAS 1965) MODELS), DIFF(HD 28344), T(B-V), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTMAA, (L) ======================================================================== HD 28992 HYADES 97 F8 AR 04 31.7 DEC +15 24 MV = 7.94 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 29139 ALF TAU K5III (EMISS H+K) AR 04 33.0 DEC +16 25 MV = 0.85 FE/H = 0 R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ (173) VAN PARADIJS, J., MEURS, E.J.A. 1974: ASTRON.ASTROPHYS. 35, 225 ........................................................................ OBSERV. : PG, 4560-5270A, 5340-5670A, 5880-6520A, 1.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 1400:, LLWW: VAN PARADIJS 1974: A+A SUPPL. 18, 447 ANALYSIS: LTE(CARBON, GINGERICH 1969), DIFF(ALF BOO), T(RIKL, SCAN 4625-5425A, ANGULAR DIAM., FE I EXCITATION), G(IONIZATION FE, CR, V, TI, SC) REMARKS : COMMENTS: CLASS : DTGMAA ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 7 A/MM INSTRUM.: OHP LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R ------------------------------------------------------------------------ (382) KOVACS, N. 1982: ASTRON.ASTROPHYS. 120, 21 ........................................................................ OBSERV. : PG, 4700-6100A, 3.3 A/MM INSTRUM.: ESO 1.5M LINELIST: LLWW, 415: ANALYSIS: DIFF(SUN), LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19 ) T(UBVRIJKL, 52,56,63,72,80,86) G(FEI/II IONIZATION) REMARKS : FINDS LITTLE EVIDENCE FOR NLTE EFFECTS COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 29310 HYADES 102 G0 AR 04 34.7 DEC +15 03 MV = 7.54 FE/H = 0 (I) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (I) ======================================================================== HD 29574 BD -13 942 K0 (WEAK METALS) AR 04 36.6 DEC -13 27 MV = 8.33 FE/H = ---- R ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE, SINGER CAMERA LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 30455 BD +18 734 G2V... AR 04 45.8 DEC +18 38 MV = 6.97 FE/H = 0 I ------------------------------------------------------------------------ ( 29) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1960: ASTROPHYS.J. 132, 553 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, LLWW: HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, I ======================================================================== HD 30495 58 ERI G2.5V AR 04 45.4 DEC -17 01 MV = 5.50 FE/H = 0 (L) ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA PROFILE), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), (L) ======================================================================== HD 30562 HR 1536 F8V AR 04 46.1 DEC -05 45 MV = 5.77 FE/H = 0 (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 30614 ALF CAM O9.5IAE AR 04 49.0 DEC +66 16 MV = 4.29 FE/H = 0 (L) ------------------------------------------------------------------------ (376) TAKADA, M. 1977: PUB.ASTRON.SOC.JAPAN 29, 439 ........................................................................ OBSERV. : PG, 3510-6660A, 4+10+20 A/MM INSTRUM.: OKAYAMA OBS. 1.9M, COUDE LINELIST: LLWW, 100: ANALYSIS: LTE(ATLAS), T+G(WIDTHS OF HGAMMA, HDELTA, HEPSILON; BALMER JUMP; N II/III, SI III/IV IONIZATION; U B C0), F-VALUES: VARIOUS SOURCES (1964-1971) AS LISTED, CHECKS: SCAN 3200-8060A, PROFILES OF HGAMMA, HDELTA, HEPSILON, HE I 4471, 4026, 3820, 4388, 4144, 4009 A HE II 5412, 4542 A REMARKS : OBSERVATIONAL DATA IS ALSO COMPARED RESULTS FROM NLTE/L MODELS (MIHALAS 1972-1975) COMMENTS: CLASS : TGM(N)AA, (L) ======================================================================== HD 30649 BD +45 992 G1V-VI AR 04 48.0 DEC +45 45 MV = 6.97 FE/H = - I ------------------------------------------------------------------------ ( 31) WALLERSTEIN, G., HELFER, H.L. 1961: ASTROPHYS.J. 133, 562 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 120:, LLWW: ( 29) HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE( IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, LLWW: ( 29) HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, I ======================================================================== HD 30652 PI3 ORI F6V (SUBDWARF) AR 04 47.1 DEC +06 53 MV = 3.19 FE/H = 0 R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (244) GRABOWSKI, B. 1976: ACTA ASTRON. 26, 147 ........................................................................ OBSERV. : PG, 3600-4500A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG(WEIGHTING FUNCTIONS FROM LTE(CAYREL, JUGAKU) MODELS; COG SHAPE FROM SUN(COWLEY'S 1964: AP.J. 140, 713), UNSOELD 1968: STERNATMOSPHAEREN), DIFF(HD 140283, SUN), T(FE I EXCITATION; TI I/II IONIZATION, NE FROM BALMER LINES VIA INGLIS-TELLER FORMULA; HGAMMA PROFILE), F-VALUES: VARIOUS WORKS(1964-1975) AS LISTED REMARKS : COMMENTS: CLASS : DTMAA, L ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : CHAFFEE 1970: A+A 4, 291; POWELL 1971: ROY.OBS.BULL. 167 INSTRUM.: LINELIST: 18 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 30676 HYADES 119 F8 AR 04 47.5 DEC +17 07 MV = 7.12 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 30810 HYADES 122 F6V AR 04 48.4 DEC +10 59 MV = 6.76 FE/H = 0 (L) ------------------------------------------------------------------------ ( 23) CHAFFEE, F.H., CARBON, D.F., STROM, S.E. 1971: ASTROPHYS.J. 166, 593 ........................................................................ OBSERV. : PG, 4325-4950A, 9+10 A/MM INSTRUM.: LICK? LINELIST: LW, 24 FE I LINES ANALYSIS: LTE(STROM), T(B-Y), G(MASS-LUMINOS.REL.==> ADOPTED), F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TMA, (L) ======================================================================== HD 31398 IOT AUR K3II (EMISS H+K) AR 04 53.7 DEC +33 05 MV = 2.70 FE/H = 0 I ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA, I ======================================================================== HD 32034 RMC 62 B:IA:... AR 04 55.2 DEC -67 15 MV = 9.68 FE/H = -- I ------------------------------------------------------------------------ (213) PRZYBYLSKI, A. 1971: MONTHLY NOT.ROY.ASTRON.SOC. 152, 197 ........................................................................ OBSERV. : PG, 3665-5041A, 10.2 A/MM INSTRUM.: MT.STROMLO, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(ETA LEO, 13 MON), THEOR. COG: WRUBEL 1949: AP.J. 109, 66 T+PE(EXCITATION+IONIZATION FE, MG, CA, TI, CR) REMARKS : COMMENTS: CLASS : DTGAA, I ======================================================================== HD 32068 ZET AUR K4IB-II+... AR 04 59.0 DEC +41 00 MV = 3.75 FE/H = 0 R ------------------------------------------------------------------------ (277) LUCK, R.E. 1977: ASTROPHYS.J. 218, 752 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MC.DONALD 2.1M, COUDE LINELIST: ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR. COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM (277) LUCK 1977: AP.J. 218, 752 INSTRUM.: SEE ALSO: AP.J. 212, 797 LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 32147 HR 1614 K3V (EMISS H+K) AR 04 58.3 DEC -05 49 MV = 6.22 FE/H = 0 R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7+9.0+16.3 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), THEOR. COG FROM LTE MODELS(PEYTREMANN 1970), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 32537 9 AUR F0V AR 05 02.8 DEC +51 32 MV = 5.00 FE/H = 0 (I) ------------------------------------------------------------------------ ( 88) PROVOST, J., VAN'T VEER-MENNERET, C. 1969: ASTRON.ASTROPHYS. 2, 218 ........................................................................ OBSERV. : PG, 3860-6650A, 9.9 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 400: ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS(MIHALAS 1965), T(HBETA, HGAMMA; EXCITATION), G(IONIZATION FE, TI, V, CR) REMARKS : COMMENTS: CLASS : DTGMAA, (I) ======================================================================== HD 32923 104 TAU G4V AR 05 04.5 DEC +18 35 MV = 5.00 FE/H = 0 (I) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (I) ======================================================================== HD 33256 68 ERI F2V AR 05 06.2 DEC -04 31 MV = 5.10 FE/H = - R ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 33299 BD +30 804 K1IB AR 05 07.4 DEC +30 44 MV = 6.69 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 33579 RMC 76 A4IA AR 05 06.0 DEC -67 57 MV = 9.11 FE/H = 0 L ------------------------------------------------------------------------ (129) PRZYBYLSKI, A. 1968: MONTHLY NOTICES ROY.ASTRON.SOC. 139, 313 ........................................................................ OBSERV. : PG, 3600-5060A, 10.2 A/MM INSTRUM.: MT.STROMLO, COUDE LINELIST: LLWW, 500: ANALYSIS: COG, DIFF(ALF CYG), THEOR.COG FROM WRUBEL 1949: AP.J.109, 66 T+PE(THREE ADOPTED SETS OF VALUES) REMARKS : COMMENTS: CLASS : DAA, I ------------------------------------------------------------------------ (185) WOLF, B. 1972: ASTRON.ASTROPHYS. 20, 275 ........................................................................ OBSERV. : PG, 3390-4950A, 12.3 A/MM INSTRUM.: ESO 1.5M, LINELIST: LLWW, 250 ANALYSIS: LTE(UNBLANKETED), T+G(BALMER JUMP; WIDTHS OF HDELTA, H8; IONIZATION MG, FE; COG OF FE, TI), CHECKED WITH SCAN 3300-5550A, F-VALUES: VARIOUS SOURCES AS QUOTED REMARKS : ALSO COMPARES LINE PROFILES OF HALFA, HDELTA, CA II K, SI II 3856+3863 A, MG II 4481 A WITH COMPUTED ONES COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ (103) PRZYBYLSKI, A., BURNICKI, A. 1974: ACT.ASTRON. 24, 275 ........................................................................ OBSERV. : PG, 3700-4924A, 10.2 A/MM INSTRUM.: MT.STROMLO LINELIST: ANALYSIS: COG, DIFF(ALF CYG, HD 67456), T(ADOPTED), PE(FE IONIZATION) REMARKS : COMMENTS: CLASS : DAA, I ======================================================================== HD 33793 KAPTEYN'S STAR M1PVAR... (SUBDWARF) AR 05 09.7 DEC -45 00 MV = 8.89 FE/H = - (R) ------------------------------------------------------------------------ (257) MOULD, J.R. 1976: ASTROPHYS.J. 210, 402 ........................................................................ OBSERV. : PG, 8400-8800A, 10+40 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE, IT LINELIST: LW, 17 ANALYSIS: LTE(MOULD 1976), DIFF(Y 5584) T(MOULD 1976: AP.J. 208, 399 (7520-10235A COLOUR, MASS- LUMINOSITY REL.)), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DA, (R) ======================================================================== HD 34255 HR 1720 K4IAB: AR 05 15.7 DEC +62 36 MV = 5.61 FE/H = 0 (I) ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA, (I) ======================================================================== HD 34334 16 AUR K2.5IIIB (EMISS H+K) AR 05 14.9 DEC +33 19 MV = 4.54 FE/H = - R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.4+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ======================================================================== HD 34411 LAM AUR G1.5IV-V AR 05 15.6 DEC +40 03 MV = 4.70 FE/H = 0 R ------------------------------------------------------------------------ ( 29) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1960: ASTROPHYS.J. 132, 553 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTGAA ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, LLWW: HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3300-4700A, 9+13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y, SCAN) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (287) KOVACS, N., FOY, R. 1978: ASTRON.ASTROPHYS. 68, 27 ........................................................................ OBSERV. : DATA FROM ( 29) HELFER ET AL.1960: AP.J. 132, 553 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM MODELS LTE(PEYTREMANN 1974)), DIFF(SUN), T(R-I), G(IONIZATION FE I/II), F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: GIVE FE/H RATIO ONLY CLASS : DTGMAA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 34816 LAM LEP B0.5IV AR 05 17.3 DEC -13 14 MV = 4.30 FE/H = + (L) ------------------------------------------------------------------------ (105) HARDORP, J., SCHOLZ, M. 1970: ASTROPHYS.J.SUPPL. 19, 193 ........................................................................ OBSERV. : PG, 3220-6700A, 4.3+6.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 420: ANALYSIS: LTE(MIHALAS 1965), T+G(BALMER JUMP; IONIZATION C, N, SI; HGAMMA, HDELTA PROF.) CHECKED WITH SCAN 3300-6500A, F-VALUES: VARIOUS SOURCES AS QUOTED REMARKS : ALSO COMPARE OBSERVED AND COMPUTED PROFILES OF HE I 4026, 4388, 4471 A, HE II 4686 A COMMENTS: CLASS : TGMAA, (L) ======================================================================== HD 35601 BD +29 897 M1.5IAB-B AR 05 24.0 DEC +29 53 MV = 7.35 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(ABS.MAG, EVOL.TRACKS) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 35620 PHI AUR K3IIICN+... (CN) AR 05 24.3 DEC +34 26 MV = 5.07 FE/H = 0 R ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : PG, 4400-6800A, 9.7+12.4 A/MM, 0.3A INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(EPS VIR), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : COMMENTS: CLASS : DTGMAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN REF.(41) INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY REF.(41) DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : PG, 4900-6600A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: LTE(ALTAS; CARBON, GINGERICH), DIFF(MEAN OF: GAM TAU, DEL TAU, EPS TAU, EPS VIR), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ ( 99) BLANC-VAZIAGA, M.-J., CAYREL , G., CAYREL, R. 1973: ASTROPHYS.J. 180, 871 ........................................................................ OBSERV. : PG, ??? , 6.8 A/MM, 0.2 A INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1970)), DIFF(EPS VIR), T+G(R-I, V-K; IONIZATION FE I/II, TI I/II, CR I/II; ABUNDANCE FROM WEAK AND STRONG LINES; ABSOLUTE MAG.) F-VALUES: DIFF(EPS VIR) REMARKS : ALSO COMPARE OBSERVED AND COMPUTED PROFILES OF NA I D, MG I B LINES COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 36389 119 TAU M2IAB: (EMISS H+K) AR 05 29.3 DEC +18 34 MV = 4.49 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(ABS.MAG, EVOL.TRACKS) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 36395 GJ 205 M1.5V (ME) AR 05 29.0 DEC -03 41 MV = 7.92 FE/H = + (R) ------------------------------------------------------------------------ (313) MOULD, J.R., 1978: ASTROPHYS.J. 226, 923 ........................................................................ OBSERV. : 1.5-2.5 MU, 1.5 A (= 4000-6600CM**-1, 0.3 CM**-1) INSTRUM.: KPNO 4M, FTS LINELIST: LW, 22 ANALYSIS: LTE(MOULD 1976), SPECTRUM SYNTHESIS, T(7540-10175 COLOUR), F-VALUES: DIFF(SUN), THEORETICAL VALUES REMARKS : COMMENTS: CLASS : (D)TMSA, (R) ======================================================================== HD 37043 B IOT ORI B B2 AR 05 33.0 DEC -05 56 MV = ? FE/H = ? (I) ------------------------------------------------------------------------ (143) CONTI, P.S., LOONEN, J.P. 1970: ASTRON.ASTROPHYS. 8, 197 ........................................................................ OBSERV. : PG, 3790-4710A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(HD 35912), THEOR.COG OF HUMMER 1968: MNRAS 138, 73 T(SAME AS HD 35912), COMPARE HGAMMA PROFILE WITH LTE MODELS(MIHALAS 1965) REMARKS : HE-WEAK STAR COMMENTS: REFERENCE STAR HD 35912 HAS NOT YET BEEN ANALYZED CLASS : D(M)AA, (I) ======================================================================== HD 37128 EPS ORI B0IAB: AR 05 33.7 DEC -01 14 MV = 1.70 FE/H = ? (I) ------------------------------------------------------------------------ (A02) LAMERS, H.J. 1972: ASTRON.ASTROPHYS. 17, 34 ........................................................................ OBSERV. : PG, 3550-6720A, 2.3-4.4 A/MM INSTRUM.: KPNO 84-INCH, ESO 1.5M, COUDE LINELIST: 200:, LLWW: LAMERS 1972: A+A SUPPL. 7, 113 ANALYSIS: COG(THEOR.COG FROM UNSOELD 1955: STERNATMOSPHAEREN), T(EXCITATION, IONIZATION+INGLIS-TELLER ON H20), F-VALUES: WIESE 1966+1969 REMARKS : ABUNDANCES OF HE, C, N, O, NE, MG, SI, S COMMENTS: CLASS : TAA, (I) ======================================================================== HD 37160 PHI2 ORI K0IIIB (EMISS H+K, S) AR 05 34.1 DEC +09 16 MV = 4.09 FE/H = - L ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN AND ATOMIC LINES WEAK COMMENTS: CLASS : (D)A, I ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (184) BACJAR, R. 1969: CONTR.ASTRON.OBS.SKALNATE PLESO 4, 63 ........................................................................ OBSERV. : PG, 3300-4800A, 9+18 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(HD 188512), THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66 T(LINE EXCITATION), PE(IONIZATION TI, V, SC, Y), F-VALUES: CORLISS, BOZMAN 1962 CHECKED WITH SOLAR SPECTRUM REMARKS : COMMENTS: CLASS : DTAA, I ======================================================================== HD 37387 BD +23 982 K1IB AR 05 36.2 DEC +23 18 MV = 7.48 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 37394 HR 1925 K1V (EMISS H+K) AR 05 37.3 DEC +53 28 MV = 6.23 FE/H = 0 (R) ------------------------------------------------------------------------ (421) PERRIN, M.-N. 1983: ASTRON.ASTROPHYS. 128, 347 ........................................................................ OBSERV. : PG, 4800-5930A, 12.4 A/MM, 0.25 A, S/N=30 INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 227 ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : HALFA LINE PROFILE IS ALSO REPRODUCED COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 37763 GAM MEN K4III (EMISS H+K) AR 05 33.9 DEC -76 23 MV = 5.17 FE/H = 0 (R) ------------------------------------------------------------------------ (293) FOY, R. 1980: ASTRON.ASTROPHYS. 85, 287 ........................................................................ OBSERV. : PG, 5200?-6200?A, 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(T-TAU FROM GUSTAFSSON) ), T(R-I), G(FE I/II IONIZATION), T+G CHECKED BY: LINE PROFILES OF MG I B TRIPLET F-VALUES AS COMPILED BY FOY 1972: A+A, 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : ABUND. OF ELEMENTS OTHER THAN FE, NA, BA WERE DERIVED FROM WEAK LINES DIFFERENTIALLY TO THE SUN COMMENTS: CLASS : (D)TGMAA, (R) ======================================================================== HD 37828 BD -11 1258 K0 (WEAK METALS) AR 05 38.6 DEC -11 13 MV = 6.87 FE/H = --- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE, SINGER CAMERA LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 38247 BD +18 950 G8IAB AR 05 42.3 DEC +18 41 MV = 6.64 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 38751 132 TAU G8III (EMISS H+K, CN) AR 05 45.9 DEC +24 33 MV = 4.86 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 38899 134 TAU B9IV AR 05 46.7 DEC +12 38 MV = 4.91 FE/H = 0 (R) ------------------------------------------------------------------------ (A25) ADELMAN, S.J. 1984: MONTHLY NOTICES ROY.ASTRON.SOC. 206, 637 ........................................................................ OBSERV. : PG, ??? , 2-15.5 A/MM INSTRUM.: MT.WILSON, LICK, KPNO LINELIST: 160:, LW: MICROFICHE MN 206/1 ANALYSIS: LTE(ATLAS), DIFF(SUN), T+G(SCAN 3300-7100A, HGAMMA PROFILE), F-VALUES: BLACKWELL, KORNBLITH+BRIDGES, AND OTHERS REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 39003 NU AUR G9.5III (EMISS H+K) AR 05 48.0 DEC +39 08 MV = 3.97 FE/H = 0 (L) ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA ======================================================================== HD 39091 PI MEN G1V AR 05 41.1 DEC -80 31 MV = 5.67 FE/H = 0 (R) ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 39364 DEL LEP K0III (EMISS H+K) AR 05 49.2 DEC -20 53 MV = 3.81 FE/H = - (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN WEAK COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 39587 KHI1 ORI G0V AR 05 51.4 DEC +20 16 MV = 4.41 FE/H = 0 (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 39853 HR 2065 K5III (EMISS H+K) AR 05 52.4 DEC -11 47 MV = 5.61 FE/H = - R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 39866 HR 2066 A2II AR 05 53.4 DEC +28 56 MV = 6.32 FE/H = ? (L) ------------------------------------------------------------------------ (172) AYDIN, C. 1972: ASTRON.ASTROPHYS. 19, 369 ........................................................................ OBSERV. : PG, 3710-4860A, 12.4 A/MM INSTRUM.: OHP 1.5M, 1.9M, COUDE LINELIST: 280:, LLWW: AYDIN 1972: ASTRON.ASTROPHYS.SUPPL. 7, 331 ANALYSIS: COG, DIFF(ALF CYG), T+G(HBETA, HGAMMA, BALMER DISC.), PE(FE I/II IONIZATION, INGLIS-TELLER) F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVES FE, TI, CR ABUNDANCES ONLY COMMENTS: CLASS : DTGA, (L) ======================================================================== HD 39949 BD +27 923 G2IB AR 05 54.0 DEC +27 19 MV = 7.21 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 40136 ETA LEP F0V AR 05 54.1 DEC -14 11 MV = 3.70 FE/H = 0 (L) ------------------------------------------------------------------------ (123) SMITH, M.A. 1971: ASTRON.ASTROPHYS. 11, 325 ........................................................................ OBSERV. : PG, ???? , 8.9+17.8 A/MM INSTRUM.: KPNO 84-INCH, COUDE LINELIST: LW: SMITH 19??: A+A SUPPL. ????????? ANALYSIS: LTE(ATLAS), T+G(FE I/II LINES), REMARKS : COMMENTS: CLASS : TGMAA, (L) ======================================================================== HD 40183-1,2 BET AUR A,B A2IV+... AR 05 55.9 DEC +44 57 MV = 1.85 FE/H = 0 (R) ------------------------------------------------------------------------ (176) TOY, L.G.S. 1969: ASTROPHYS.J. 158, 1099 ........................................................................ OBSERV. : PG, 3900-4500A, 3 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 100: ANALYSIS: LTE(STROM), T(SCAN 3400-5560 A, FE I EXCITATION) G(FE I/II IONIZATION), F-VALUES: CORLISS WARNER 1964 REMARKS : FINDS ABUNDANCE PATTERN TO BE SIMILAR TO THAT OF AM STARS COMMENTS: CLASS : TGMAA, (R) ======================================================================== HD 40409 HR 2102 K1III-IV (EMISS H+K) AR 05 53.7 DEC -63 06 MV = 4.66 FE/H = 0 (R) ------------------------------------------------------------------------ (287) KOVACS, N., FOY, R. 1978: ASTRON.ASTROPHYS. 68, 27 ........................................................................ OBSERV. : PG, 5250-6200A, 12.4 A/MM INSTRUM.: ESO 1.5M LINELIST: LLWW, 280: ANALYSIS: COG(T-TAU FROM MODELS LTE(GUSTAFSSON)), DIFF(SUN), T+G(R-I, IONIZATION FE I/II, LINE PROFILES NA I D, MG I B) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 41312 HR 2140 K3III AR 06 01.2 DEC -26 17 MV = 5.06 FE/H = -- (R) ------------------------------------------------------------------------ (293) FOY, R. 1980: ASTRON.ASTROPHYS. 85, 287 ........................................................................ OBSERV. : PG, 5200?-6200?A, 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(T-TAU FROM GUSTAFSSON) ), T(R-I, V-K), G(FE I/II IONIZATION), T+G CHECKED BY: LINE PROFILES OF MG I B TRIPLET F-VALUES AS COMPILED BY FOY 1972: A+A, 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : ABUND. OF ELEMENTS OTHER THAN FE, NA, BA WERE DERIVED FROM WEAK LINES DIFFERENTIALLY TO THE SUN COMMENTS: CLASS : (D)TGMAA, (R) ======================================================================== HD 41636 HR 2153 G9III AR 06 04.9 DEC +41 04 MV = 6.36 FE/H = - (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 41692 HR 2154 B5IV AR 06 04.2 DEC -04 11 MV = 5.39 FE/H = - (R) ------------------------------------------------------------------------ (A25) ADELMAN, S.J. 1984: MONTHLY NOTICES ROY.ASTRON.SOC. 206, 637 ........................................................................ OBSERV. : PG, ??? , 4-8.9 A/MM INSTRUM.: MT.WILSON, MT.PALOMAR, LICK, KPNO LINELIST: 50:, LW: MICROFICHE MN 206/1 ANALYSIS: LTE(ATLAS), DIFF(SUN), T+G(SCAN 3300-7100A, HGAMMA PROFILE), F-VALUES: BLACKWELL, KORNBLITH+BRIDGES, AND OTHERS REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 42454 BD +29 1140A G2IB AR 06 08.9 DEC +29 30 MV = 7.32 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 42474 WY GEM M2IABPE AR 06 08.9 DEC +23 13 MV = 7.21 FE/H = - (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(ABS.MAG, EVOL.TRACKS) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 42475 HR 2190 M1IAB: AR 06 08.8 DEC +21 53 MV = 6.6 FE/H = - (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(ABS.MAG, EVOL.TRACKS) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 42543 6 GEM M1 AR 06 09.3 DEC +22 55 MV = 6.39 FE/H = - (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(ABS.MAG, EVOL.TRACKS) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 42581 GJ 229 M1V AR 06 08.5 DEC -21 51 MV = 8.14 FE/H = 0 (R) ------------------------------------------------------------------------ (313) MOULD, J.R., 1978: ASTROPHYS.J. 226, 923 ........................................................................ OBSERV. : 1.5-2.5 MU, 1.5 A (= 4000-6600CM**-1, 0.3 CM**-1) INSTRUM.: KPNO 4M, FTS LINELIST: LW, 22 ANALYSIS: LTE(MOULD 1976), SPECTRUM SYNTHESIS, T(7540-10175 COLOUR), F-VALUES: DIFF(SUN), THEORETICAL VALUES REMARKS : METALLICITY FROM AL, CA, MG COMMENTS: CLASS : (D)TMSA, (R) ======================================================================== HD 43039 KAP AUR G8.5IIIB (EMISS H+K) AR 06 12.2 DEC +29 31 MV = 4.35 FE/H = 0 L ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 43) HELFER 1968: AP.J.SUPPL. 16, 1 INSTRUM.: LINELIST: ANALYSIS: DIFF(MEAN OF GAM TAU, DEL TAU, EPS TAU, EPS VIR), LTE(ATLAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ======================================================================== HD 43153 72 ORI B7V AR 06 12.5 DEC +16 10 MV = 5.34 FE/H = - (L) ------------------------------------------------------------------------ (331) HEACOX, W.D. 1979: ASTROPHYS.J.SUPPL. 41, 675 ........................................................................ OBSERV. : PG, 3100-4700A, 6.8 A/MM, 0.14 A, MN III (1285 A) INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LLWW, 80: ANALYSIS: LTE(KPA), T(C0,M0), G(HGAMMA, HDELTA) FE F-VALUES OF WARNER(1967), CORRECTED AFTER SMITH(1976) REMARKS : GIVES ABUNDANCES FOR XI = 0 AND 3 KM/S COMMENTS: CLASS : TGMAA, (L) ======================================================================== HD 43834 ALF MEN G6V AR 06 11.7 DEC -74 44 MV = 5.09 FE/H = 0 (L?) ------------------------------------------------------------------------ (250) POWELL, J.E.F., POWELL, A.L.T., STARKEY, J.R. 1976: MONTHLY NOTICES ASTRON.SOC.SOUTH AFRICA 35, 104 ........................................................................ OBSERV. : PG, 4320-4600A, 6.8 A/MM; 5230-6570A, 13.6 A/MM INSTRUM.: RADCLIFFE OBS., COUDE LINELIST: 131 ANALYSIS: COG, DIFF(SUN), T(R-I, HALFA PROFILE) REMARKS : COMMENTS: SHORT COMMUNICATION CLASS : DTMA, (L?) ======================================================================== HD 44030 BD +25 1223 K4III AR 06 17.5 DEC +25 38 MV = 7.58 FE/H = -- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 44033 HR 2269 K3IAB: AR 06 17.2 DEC +14 40 MV = 5.69 FE/H = 0 (I) ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA, (I) ======================================================================== HD 44391 BD +28 1097 K0IB AR 06 19.6 DEC +28 01 MV = 7.74 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 44537 PSI1 AUR M0IAB: VAR (EMISS H+K) AR 06 21.0 DEC +49 19 MV = 4.9 FE/H = 0 (I) ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA, (I) ======================================================================== HD 45348 ALF CAR F0II AR 06 22.8 DEC -52 40 MV = -0.72 FE/H = 0 R ------------------------------------------------------------------------ (103) PRZYBYLSKI, A., BURNICKI, A. 1974: ACT.ASTRON. 24, 275 ........................................................................ OBSERV. : PG, 3700-4924A, 10.2 A/MM INSTRUM.: MT.STROMLO LINELIST: ANALYSIS: COG, DIFF(ALF CYG, HD 67456), T(ADOPTED), PE(FE IONIZATION) REMARKS : COMMENTS: CLASS : DAA ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5300-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (409) DESIKACHARY, K., HEARNSHAW, J.B. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 707 ........................................................................ OBSERV. : PG, 3060-6850A, 2 A/MM, 0.1 A INSTRUM.: MT.JOHN 0.6M, CASSEGRAIN, ECHELLE LINELIST: 1506, LLWW: HEARNSHAW 1982: MNRAS 198, 311 AND MICROFICHE MN 198/1 ANALYSIS: LTE(ATLAS), T(UBVRI, UVBY, SCAN 3000-8080A, ANGULAR DIAM.) G(UVBY; HGAMMA, HDELTA PROFILES), REMARKS : GIVE ABUNDANCES RELATIVE TO THOSE OF THE SUN WHICH HAD BEEN OBTAINED WITH THE SAME F-VALUES AS USED IN THIS WORK COMMENTS: CLASS : (D)TGMAA, R ======================================================================== HD 45829 BD +08 1367 K0IAB AR 06 27.3 DEC +07 57 MV = 6.63 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 46300 13 MON A0IB AR 06 30.2 DEC +07 22 MV = 4.50 FE/H = - (I) ------------------------------------------------------------------------ (115) PRZYBYLSKI, A. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 146, 71 ........................................................................ OBSERV. : PG, 3670-6563A, 10.2+20.4 A/MM INSTRUM.: MT.STROMLO, COUDE LINELIST: LLWW, 550:, USED FOR ANALYSIS: 304 ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949) T+PE(FE IONIZATION) REMARKS : COMMENTS: CLASS : TAA, (I) ======================================================================== HD 47105 GAM GEM A0IV AR 06 34.8 DEC +16 27 MV = 1.90 FE/H = ? R ------------------------------------------------------------------------ ( 65) STROM, S.E., STROM, K.M. 1966: ASTRON.J. 71, 181 ........................................................................ OBSERV. : DATA FROM WRIGHT ET AL.1964: PUBL.DOMINION AP.OBS. 12, 173 INSTRUM.: LINELIST: ANALYSIS: LTE(STROM ET AL.1965: ASTRON.J. 70, 148) REMARKS : COMMENTS: SHORT COMMUNICATION CLASS : MAA ------------------------------------------------------------------------ (190) SEARLE, L., LUNGERSHAUSEN, W., SARGENT, W.L.W. 1966: ASTROPHYS.J. 145, 141 ........................................................................ OBSERV. : PG, 3200-3600A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 29 ANALYSIS: COG, DIFF(OMI PEG), THEOR.COG FROM WRUBEL 1949 T(TI II EXCITATION), F-VALUES: CORLISS, BOZMAN 1962 REMARKS : DERIVE ABUNDANCES OF FE, CR, MN, TI COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (145) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 154, 975 ........................................................................ OBSERV. : PG, 3300-6250A, 4.5+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 300: ANALYSIS: LTE(STROM), T+G(FE I EXCITATION, FEI/II IONIZATION) REMARKS : COMMENTS: BVI COLOURS ARE NOT EXPLICITLY COMPARED WITH MODEL COLOURS CLASS : TGMAA, L ------------------------------------------------------------------------ (395) SADAKANE, K., NISHIMURA, M. 1979: PUBL.ASTRON.SOC.JAPAN 31, 481 ........................................................................ OBSERV. : PG, 3610-4900A, 4+5.6 A/MM INSTRUM.: OKAYAMA OBS. 1.9M, COUDE LINELIST: LLWW, 110: ANALYSIS: LTE(ATLAS), DIFF(ALF LYR), T(CODE ET AL.1976: AP.J. 203, 417) F-VALUES: SAME AS LISTED BY SADAKANE 1976: PASJ, 28, 469 REMARKS : COMMENTS: CLASS : DMAA, R ======================================================================== HD 47205 NU2 CMA K1IV (EMISS H+K) AR 06 34.5 DEC -19 13 MV = 3.96 FE/H = 0 (R) ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, (R) ======================================================================== HD 47731 25 GEM G5IB AR 06 38.2 DEC +28 15 MV = 6.42 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 48329 EPS GEM G8IB VAR (EMISS H+K) AR 06 40.9 DEC +25 11 MV = 2.98 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 5000-6650A, 1.6 A/MM INSTRUM.: MT.WILSON 100-INCH LINELIST: 800:, LLWW: VAN PARADIJS 1973: A+A SUPPL. 11, 25 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(SUN, EPS VIR), THEOR.COG FROM HSRA(SUN) AND LTE MODELS(GUSTAFSSON) T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 48640 BD +24 1386 K2:IB AR 06 42.3 DEC +24 44 MV = 7.0 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 48781 PSI6 AUR K1III AR 06 43.8 DEC +48 51 MV = 5.22 FE/H = 0 L ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : PG, 4400-6800A, 9.7+12.4 A/MM, 0.3A INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(EPS VIR), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (380) KOMAROV, N.S., SHCHERBAK, A.N. 1980: SOVIET ASTRON. 24, 323 ........................................................................ OBSERV. : DATA FROM CAYREL DE STROBEL 1966: ANN.ASTROPHYS. 5, 413 INSTRUM.: CRIMEAN AP.OBS. 50-INCH LINELIST: ANALYSIS: COG, DIFF(ALF BOO), T(FE I EXCITATION), PE(FE I/II IONZATION) REMARKS : COMMENTS: CLASS : DTAA, L ======================================================================== HD 49009 NGC 2281 63 K2 AR 06 44.8 DEC +41 22 MV = 7.26 FE/H = - (L) ------------------------------------------------------------------------ ( 12) WALLERSTEIN, G., CONTI, P.S. 1964: ASTROPHYS.J. 140, 858 ........................................................................ OBSERV. : PG, 5000-6600A, 13.5-16.0 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH,LICK 120-INCH, COUDE LINELIST: LLWW, 216 ANALYSIS: COG, DIFF(GAM TAU), T(FE I, TI I EXCITATION, UVBGRI), REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 49068 NGC 2287 75 K1.5II-III AR 06 43.6 DEC -20 48 MV = 7.44 FE/H = - (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA ======================================================================== HD 49091 NGC 2287 21 K2 AR 06 43.8 DEC -20 43 MV = 6.90 FE/H = 0 (I) ------------------------------------------------------------------------ ( 1) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1959: ASTROPHYS.J. 129, 700 ........................................................................ OBSERV. : PG, 4000-4900A, 9+18 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG(WRUBEL 1949), DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, (I) ======================================================================== HD 50778 TET CMA K4III (EMISS H+K) AR 06 51.9 DEC -11 58 MV = 4.05 FE/H = 0 R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.4+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ======================================================================== HD 50877 OMI1 CMA K2IAB (EMISS H+K) AR 06 52.0 DEC -24 07 MV = 3.87 FE/H = 0 R ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 52005 41 GEM K4IAB (EMISS H+K) AR 06 57.4 DEC +16 09 MV = 5.68 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 52711 HR 2643 G4V AR 07 00.3 DEC +29 25 MV = 5.93 FE/H = 0 (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 54605 DEL CMA F8IAB: AR 07 06.4 DEC -26 19 MV = 1.80 FE/H = 0 R ------------------------------------------------------------------------ (153) BELL, R.A., RODGERS, A.W. 1965: MONTHLY NOTICES ROY.ASTRON.SOC. 129, 127 ........................................................................ OBSERV. : PG, 3865-4730A, 2.3 A/MM INSTRUM.: MT.STROMLO 74-INCH, COUDE LINELIST: LLWW, 130: FE LINES ANALYSIS: COG(WRUBEL 1949), T(FE I EXCITATION), F-VALUES: CORLISS, BOZMAN 1962 REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : TA ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5300-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (423) LUCK, R.E., LAMBERT, D.L. 1981: ASTROPHYS.J. 245, 1018 ........................................................................ OBSERV. : PE, RETICON, 100A SECTIONS CENTERED AT 5380, 6300, 6385, 6425, 6560, 8710A, 0.2A, S/N=100 INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: DOAR, 150-250 ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: GIVE ABUNDANCES FOR C, N, O, FE CLASS : DTGMSA, R ======================================================================== HD 55575 HR 2721 G0V AR 07 12.1 DEC +47 20 MV = 5.60 FE/H = - R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 56224 BD +26 1510 K1III AR 07 14.2 DEC +26 27 MV = 7.25 FE/H = - (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-V), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 56577 HR 2764 K3IB (EMISS H+K) AR 07 14.5 DEC -23 14 MV = 4.79 FE/H = 0 R ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 58207 IOT GEM G9IIIB (COMPOSITE, EMISS H+K) AR 07 22.6 DEC +27 54 MV = 3.79 FE/H = 0 (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 58343 HR 2825 B2.5IVE AR 07 22.6 DEC -16 06 MV = 5.33 FE/H = + R ------------------------------------------------------------------------ (106) KODAIRA, K., SCHOLZ, M. 1970: ASTRON.ASTROPHYS. 6, 93 ........................................................................ OBSERV. : PG, 3448-6678A, 4.3+6.5+10.4+15.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 35: ANALYSIS: LTE(UNBLANKETED: MIHALAS, STROM+AVRETT), DIFF(IOT HER), T+G(BJ; IONIZATION SI II/III; BALMER LINE WINGS), F-VALUES: VARIOUS SOURCES AS LISTED COMPARE OBS.AND CALC. PROFILES OF HALFA..HDELTA, HE I 4471, 4026, 4388 A, SCAN 3300..7000 A REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 58551 HR 2835 F6V AR 07 23.9 DEC +21 38 MV = 6.54 FE/H = -- (R) ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3800-4700A, 9 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y, SCAN) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, (R) ======================================================================== HD 60778 BD +00 2011 A1V (HOR.BRANCH) AR 07 33.6 DEC -00 01 MV = 9.10 FE/H = - (R?) ------------------------------------------------------------------------ (379) DANFORD, S.C., LEA, S.M. 1981: ASTRON.J. 86, 1909 ........................................................................ OBSERV. : PG, 4850-4700A, 16.9 A/MM INSTRUM.: KPNO 2.1M, COUDE LINELIST: LW, 46 ANALYSIS: LTE(ATLAS), T+G(SCAN: DANFORD 1976: THESIS, YALE UNIV.) F-VALUES: VARIOUS SOURCES (1969-78) LISTED REMARKS : COMMENTS: CLASS : MAA, (R?) ======================================================================== HD 61421 ALF CMI F5IV (EMISS H+K) AR 07 36.7 DEC +05 21 MV = 0.38 FE/H = 0 R ------------------------------------------------------------------------ (156) GREENSTEIN, J.L. 1948: ASTROPHYS.J. 107, 151 ........................................................................ OBSERV. : PG, 4010-4830A, 2.8 A/MM INSTRUM.: MCDONALD, COUDE LINELIST: LLWW, 350 ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (167) WRIGHT, K.O. 1951: PUBL.DOM.ASTROPHYS.OBS.VICTORIA 8, 1 ........................................................................ OBSERV. : PG, 3700-6750A, 4.8...20.8 A/MM INSTRUM.: DAO 72-INCH, CASSEGRAIN LINELIST: LLWW, 800 ANALYSIS: COG, DIFF(SUN), THEO.COG MENZEL, UNSOELD 1936: AP.J. 84, 474 T(FE I, TI I EXCITATION) REMARKS : COMMENTS: OBSERVATIONS WERE DONE BETWEEN 1937-1945 CLASS : DTAA ------------------------------------------------------------------------ ( 48) EDMONDS, F.N. 1965: ASTROPHYS.J. 142, 278 ........................................................................ OBSERV. : PG, 3170-6680A, 3.2+4.8+9.6 A/MM INSTRUM.: MCDONALD 82-INCH, COUDE LINELIST: LLWW, 152 ANALYSIS: REMARKS : ALSO MEASURES LINE PROFILES OF HALFA, HBETA, CA II K COMMENTS: NO DERIVATION OF ABUNDANCES FROM SPECTRAL DATA CLASS : ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 84) GRIFFIN, R. 1971: MONTHLY NOTICES ROY.ASTRON.SOC. 155, 139 ........................................................................ OBSERV. : PG, 3375-7500A, 1 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(FE, TI, SI, CR, NI EXCITATION) REMARKS : PRELIMINARY ANALYSIS COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (238) HASEGAWA, T. 1975: SENDAI ASTRON.RAP. 164 ........................................................................ OBSERV. : PG, 4000-6000A, ??? A/MM INSTRUM.: OKAYAMA 74-INCH LINELIST: LLWW, 250:, CF. HASEGAWA 1973: J.HOKKAIDO UNIV.EDUC. II B 23, 90 ANALYSIS: COG(THEO.COG WRUBEL 1949: AP.J. 109, 66) T(LINE EXCITATION), F-VALUES: VARIOUS SOURCES LISTED REMARKS : CONSIDERS FE I,II, TI I,II, CR I, NI I COMMENTS: CLASS : TA ------------------------------------------------------------------------ (291) TOMKIN, J., LAMBERT, D.L., 1978: ASTROPHYS.J. 223, 937 ........................................................................ OBSERV. : PE, 100A SECTIONS IN THE RANGE 6500-9300A, 0.2A, S/N= 500 INSTRUM.: MCDONALD 2.7M, COUDE, SI PHOTODIODE ARRAY LINELIST: LW, 56: ANALYSIS: LTE(ATLAS), T+G(B-Y, C1; BETA), G(BINARY SYSTEM), F-VALUES: DIFF(SUN, HOLWEGER-MUELLER MODEL), THEORETICAL REMARKS : DERIVE C, N, O, FE ABUNDANCES COMMENTS: CLASS : (D)TA, R ------------------------------------------------------------------------ (386) KATO, K., SADAKANE, R. 1982,: ASTRON.ASTROPHYS. 113, 135 ........................................................................ OBSERV. : DATA FROM GRIFFIN, GRIFFIN 1979: A PHOTOMETRIC ATLAS OF THE SPECTRUM OF PROCYON, CAMBRIDGE, ENGLAND INSTRUM.: LINELIST: LLWW, 360: ANALYSIS: LTE(ATLAS), DIFF(SUN), T(SCAN 3300-10000A; PROFILES OF HALFA, HBETA, HGAMMA; BETA; B-Y; IONIZATION OF SI, CA, TI, CR, FE), G(BINARY SYSTEM, ANGULAR DIAMETER, IR FLUX), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 62345 KAP GEM G8IIIA (EMISS H+K) AR 07 41.6 DEC +24 31 MV = 3.57 FE/H = 0 I ------------------------------------------------------------------------ ( 15) BURBIDGE, E.M., BURBIDGE, G.R. 1957: ASTROPHYS.J. 126, 357 ........................................................................ OBSERV. : PG, 4200-6800A, 10+15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 1200: ANALYSIS: COG, DIFF(SUN), THEOR.COG: WRUBEL 1949: AP.J. 109, 66 T(FE I EXCITATION) REMARKS : USE STAR AS REFERENCE FOR STUDY OF A BA STAR COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : COMMENTS: CLASS : (D)A, I ======================================================================== HD 62509 BET GEM K0IIIB (EMISS H+K) AR 07 42.3 DEC +28 09 MV = 1.14 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (242) GRIFFIN, R. 1976: MONTHLY NOTICES ROY.ASTRON.SOC. 175, 225 ........................................................................ OBSERV. : PG, 5580-6330A, 1.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 650: ANALYSIS: COG, DIFF(ALF BOO), T(RIJK) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (339) RULAND, F., HOLWEGER, H., GRIFFIN, R. AND R., BIEHL, D. 1980: ASTRON.ASTROPHYS. 92, 70 ........................................................................ OBSERV. : PG, 3780-7500A, 1+1.5 A/MM; 5115-5215A, 8530-8735A, INSTRUM.: MT.WILSON 100-INCH, COUDE ; KPNO 1.5M MCMATH, FTS LINELIST: LLWW: RULAND ET AL.1980: ASTRON.ASTROPHYS.SUPPL. 42, 391 ANALYSIS: EMPIRICAL LTE MODEL DERIVED FROM LINE WINGS OF MG B, NA D, CA II 8542+8662 CHECKED WITH CA II H+K, CA I 4226, FE I 4383 ALSO LTE(GUSTAFSSON) T(SCAN 5200-11000A, VRIJK), G(FE IONIZATION), F-VALUES: DIFF(SUN, HOLEGER-MUELLER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ------------------------------------------------------------------------ (426) TOMKIN, J., LAMBERT, D.L. 1983: ASTROPHYS.J. 273, 722 ........................................................................ OBSERV. : PE, DIGICON: 20A SECTIONS FROM 4000-5300A, 0.04A, RETICON: 20A SECTIONS FROM 5300-8000A, 0.09A, S/N= 100 INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, DIGICON, RETICON LINELIST: LW, 100: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T(R-I), G(FE IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 62576 1 PUP K5III AR 07 41.5 DEC -28 17 MV = 4.59 FE/H = 0 R ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 62644 HR2998 G6IV AR 07 41.6 DEC -45 03 MV = 5.04 FE/H = - (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 63077 HR3018 G0V (SUBDWARF) AR 07 43.7 DEC -34 04 MV = 5.37 FE/H = -- R ------------------------------------------------------------------------ ( 32) KONDO, M. 1957: PUBL.ASTRON.SOC.JAPAN 9, 201 ........................................................................ OBSERV. : PG, 4060-4810A, 11+15 A/MM INSTRUM.: LICK 36-INCH LINELIST: LLWW, 220: ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM WRUBEL 1949, T(HGAMMA EQ.WIDTH, LEAST SCATTER ON COG) REMARKS : COG CONSTRUCTED ONLY FROM FE LINES, ABUNDANCES ARE DERIVED ROUGHLY FROM THE EQ.WIDTH DIFFERENCES OF STAR AND STANDARD COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 71) BUTCHER, H.R. 1972: ASTROPHYS.J. 176, 711 ........................................................................ OBSERV. : PG, 70A RANGE AT 4130A, 1 A/MM, 0.08A INSTRUM.: MT.STROMLO 1.9M, COUDE, ECHELLE, IT LINELIST: LW, 3 ANALYSIS: COG(15 FE I LINES, SOLAR COG, MILNE-EDDINGTON ATMOSPHERE), T(COG SHIFTS REL.TO MODELS OF CAYREL+JUGAKU 1963) REMARKS : PRESENTS PRELIMINARY RESULTS OF LARGER SURVEY CONSIDERS BA II 4130, EU II 4129, FE II 4128 ONLY COMMENTS: CLASS : DT(M)A ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (191) DA SILVA, L. 1975: ASTRON.ASTROPHYS. 41, 287 ........................................................................ OBSERV. : PG, 4390-6600A, 3.2+12.4 A/MM, 0.14+0.30 A INSTRUM.: ESO 1.5M, COUDE LINELIST: DAOR, 400: ANALYSIS: LTE(PEYTREMANN 1970), DIFF(SUN), T(B-Y, R-I, BETA; WINGS OF HALFA, HBETA), T+G(PARALLAXES, MASS-LUMINOSITY REL.; IONIZATION FE, CR, TI), REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I, SCAN), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3800-4700A, 9 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 63302 HR 3026 K1IA-AB AR 07 45.4 DEC -15 52 MV = 6.34 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 63700 XI PUP G6IAB (EMISS H+K) AR 07 47.2 DEC -24 44 MV = 3.40 FE/H = 0 R ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 63791 BD +62 959 G0 (WEAK METALS) AR 07 50.1 DEC +62 16 MV = 8.2 FE/H = --- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 64090 BD +31 1684A G2VI (SUBDWARF) AR 07 50.4 DEC +30 46 MV = 8.30 FE/H = --- R ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : PG, 4500-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, EGC LINELIST: LLWW, 50: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), LTE(ATLAS), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 120: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: SUPERSEDED BY (309) PETERSON 1980: AP.J. 235, 491 CLASS : DTGMA ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : DATA FROM (245) HEARNSHAW 1976: A+A 51, 71 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION) REMARKS : REANALYSIS COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-4620A, 1.48 A/MM, 0.18 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 120:, LLWW: PETERSON 1978: ASTROPHYS.J. 222, 181 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL, CA, TI ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA, R ======================================================================== HD 65583 BD +29 1664 G8V AR 07 57.4 DEC +29 22 MV = 6.94 FE/H = -- R ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : PG, 4500-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, EGC LINELIST: LLWW, 150: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), LTE(ATLAS), DIFF(SUN) T(R-I), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : DATA FROM (245) HEARNSHAW 1976: A+A 51, 71 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION) REMARKS : REANALYSIS COMMENTS: CLASS : DGMA, R ======================================================================== HD 68879 NGC 2548 8???? G8III AR 08 11.8 DEC -05 45 MV = 8.20 FE/H = - (L) ------------------------------------------------------------------------ ( 12) WALLERSTEIN, G., CONTI, P.S. 1964: ASTROPHYS.J. 140, 858 ........................................................................ OBSERV. : PG, 5000-6600A, 13.5-16.0 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH,LICK 120-INCH, COUDE LINELIST: LLWW, 216 ANALYSIS: COG, DIFF(GAM TAU), T(FE I, TI I EXCITATION, UVBGRI), REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 69897 KHI CNC F6V AR 08 17.0 DEC +27 23 MV = 5.10 FE/H = - (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 71369 OMI UMA G5III (EMISS H+K) AR 08 26.1 DEC +60 53 MV = 3.40 FE/H = 0 (R) ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: OHP LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, (R) ======================================================================== HD 71597 BD +00 2305 K2III AR 08 25.7 DEC +00 25 MV = 7.31 FE/H = - (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 72324 UPS2 CNC G9III (EMISS H+K) AR 08 30.0 DEC +24 15 MV = 6.36 FE/H = 0 (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN SLIGHTLY STRONG COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 72905 PI1 UMA G1.5VB (EMISS H+K) AR 08 34.8 DEC +65 12 MV = 5.60 FE/H = - (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 73394 BD +52 1329 G5III WS (WEAK METALS) AR 08 36.7 DEC +51 56 MV = 7.70 FE/H = --- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 5200-6800A, 2.3 A/MM, 0.1A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 73665 NGC 2632 253 G8III AR 08 37.2 DEC +20 11 MV = 6.39 FE/H = 0 (L) ------------------------------------------------------------------------ ( 12) WALLERSTEIN, G., CONTI, P.S. 1964: ASTROPHYS.J. 140, 858 ........................................................................ OBSERV. : PG, 5000-6600A, 13.5-16.0 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH,LICK 120-INCH, COUDE LINELIST: LLWW, 216 ANALYSIS: COG, DIFF(GAM TAU), T(FE I, TI I EXCITATION, UVBGRI), REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 73666 NGC 2632 265 A1V AR 08 37.3 DEC +20 09 MV = 6.6 FE/H = - L ------------------------------------------------------------------------ (223) CONTI, P.S., WALLERSTEIN, G., WING, R.F. 1965: ASTROPHYS.J. 142, 999 ........................................................................ OBSERV. : PG, 3850-6800A, 10.5+16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 400: ANALYSIS: COG(THEOR. COG FROM LTE(MIHALAS 1965) MODELS), DIFF(HD 28344), T(B-V), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTMAA, L ------------------------------------------------------------------------ ( 65) STROM, S.E., STROM, K.M. 1966: ASTRON.J. 71, 181 ........................................................................ OBSERV. : DATA FROM WRIGHT ET AL.1964: PUBL.DOMINION AP.OBS. 12, 173 INSTRUM.: LINELIST: ANALYSIS: LTE(STROM ET AL.1965: ASTRON.J. 70, 148) REMARKS : COMMENTS: SHORT COMMUNICATION CLASS : MAA ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : PG, 3930-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: LTE(UNBLANKETED), T(B-V(?), FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA, L ======================================================================== HD 73710 NGC 2632 283 G9III AR 08 37.5 DEC +19 51 MV = 6.44 FE/H = 0 (L) ------------------------------------------------------------------------ ( 12) WALLERSTEIN, G., CONTI, P.S. 1964: ASTROPHYS.J. 140, 858 ........................................................................ OBSERV. : PG, 5000-6600A, 13.5-16.0 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH,LICK 120-INCH, COUDE LINELIST: LLWW, 216 ANALYSIS: COG, DIFF(GAM TAU), T(FE I, TI I EXCITATION, UVBGRI), REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 74000 BD -15 2546 F6VI (WEAK METALS, SUBDWARF) AR 08 38.5 DEC -16 07 MV = 9.67 FE/H = ---- R ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 50: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: CLASS : DTGMA ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ======================================================================== HD 74280 ETA HYA B3V AR 08 40.6 DEC +03 35 MV = 4.30 FE/H = ? (R) ------------------------------------------------------------------------ (106) KODAIRA, K., SCHOLZ, M. 1970: ASTRON.ASTROPHYS. 6, 93 ........................................................................ OBSERV. : PG, 3448-4713A, 4.3 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 15: ANALYSIS: LTE(UNBLANKETED: MIHALAS, STROM+AVRETT), DIFF(IOT HER), T+G(BJ; IONIZATION SI II/III; BALMER LINE WINGS), F-VALUES: VARIOUS SOURCES AS LISTED COMPARE OBS.AND CALC. PROFILES OF HGAMMA, HDELTA, SCAN 3300-7000 A REMARKS : FE ABUNDANCE NOT DETERMINED COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 74462 BD +67 559 G5IV (EMISS H+K, SUBDWARF) AR 08 43.8 DEC +67 38 MV = 8.74 FE/H = --- R ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 5200-6800A, 2.3 A/MM, 0.1A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 74395 HR 3459 G2IAB: (EMISS H+K) AR 08 41.2 DEC -07 03 MV = 4.62 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 75732 RHO1 CNC G8V AR 08 49.6 DEC +28 31 MV = 5.95 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 4.5+6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: SUPERSEDED BY (275) OINAS 1977: A+A 61, 17 ?? CLASS : DTGMAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: COG(LTE(PEYTREMANN 1970) MODELS), DIFF(SUN), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ======================================================================== HD 76151 HR 3538 G2V AR 08 51.8 DEC -05 15 MV = 6.00 FE/H = 0 (L) ------------------------------------------------------------------------ (324) CAYREL DE STROBEL, G., KNOWLES, N., HERNANDEZ, G., BENTOLILA, C. 1981: ASTRON.ASTROPHYS. 94, 1 ........................................................................ OBSERV. : PG, 4000-4900A, 12.4A/MM, 0.30A INSTRUM.: OHP 1.52M, COUDE LINELIST: LLWW, 210: ANALYSIS: COG, DIFF(SUN), T(B-Y, B2-V1, HBETA+HGAMMA), G(4383A) REMARKS : LOOKING FOR SOLAR TWINS COMMENTS: CLASS : DTGAA, (L) ======================================================================== HD 76294 ZET HYA G9II-III AR 08 52.8 DEC +06 08 MV = 3.11 FE/H = 0 (I) ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA, (I) ======================================================================== HD 76932 HR 3578 F6V AR 08 56.4 DEC -15 56 MV = 5.86 FE/H = --- (R) ------------------------------------------------------------------------ (281) BARBUY, B. 1978: ASTRON.ASTROPHYS. 67, 339 ........................................................................ OBSERV. : PG, 4315-4970A, 12 A/MM INSTRUM.: ESO, COUDE LINELIST: LLWW, 180: ANALYSIS: LTE(PEYTREMANN 1974), DIFF(SUN)???, T(R-I, B2-V, B-Y,BETA; HBETA PROFILE), G(TI, CR, FE IONIZATION), F-VALUES: ??? REMARKS : COMMENTS: CLASS : TGMAA, (R) ------------------------------------------------------------------------ (322) SPITE, M., SPITE, F. 1980: ASTRON.ASTROPHYS. 89, 118 ........................................................................ OBSERV. : PG, 3930-3970A, 7.1 A/MM INSTRUM.: ESO 1.5M, COUDE, ECHELLE, LALLEMAND EGC LINELIST: LW, 4 ANALYSIS: LTE(PEYTREMANN 1974, GUSTAFSSON), DIFF(SUN), T+G(BARBUY 1978: A+A 67, 339), F-VALUES: WIESE 1969 NSRDS-NBS 22 SPECTRUM SYNTHESIS REMARKS : DERIVE AL ABUNDANCE ONLY COMMENTS: FE AND MG ABUNDANCES ARE QUOTED FROM OTHER WORKS CLASS : DMSA ======================================================================== HD 77236 BD -01 2181 K0III AR 08 58.7 DEC -02 22 MV = 7.54 FE/H = 0 (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 77729 BD +26 1895 K4III AR 09 02.1 DEC +26 22 MV = 7.64 FE/H = - (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 78418 75 CNC G5IV-V AR 09 05.8 DEC +26 50 MV = 5.98 FE/H = - (L) ------------------------------------------------------------------------ (324) CAYREL DE STROBEL, G., KNOWLES, N., HERNANDEZ, G., BENTOLILA, C. 1981: ASTRON.ASTROPHYS. 94, 1 ........................................................................ OBSERV. : PG, 4000-4900A, 12.4 A/MM, 0.30A INSTRUM.: OHP 1.52M, COUDE LINELIST: LLWW, 210: ANALYSIS: COG, DIFF(SUN), T(B-Y, B2-V1, HBETA+HGAMMA), G(4383A) REMARKS : LOOKING FOR SOLAR TWINS COMMENTS: CLASS : DTGAA, (L) ======================================================================== HD 78647 LAM VEL K4IB-II AR 09 06.1 DEC -43 14 MV = 2.21 FE/H = 0 (R) ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5300-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 79452 HR 3664 G6III (EMISS H+K, WEAK METALS) AR 09 12.2 DEC +34 50 MV = 5.97 FE/H = -- (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 81192 BD +20 2318 G7III (WEAK METALS, EMISS H+K) AR 09 21.9 DEC +20 00 MV = 6.54 FE/H = -- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 5200-6800A, 2.3 A/MM, 0.1A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 81797 ALF HYA K3II-III (EMISS H+K) AR 09 25.1 DEC -08 26 MV = 1.98 FE/H = 0 (R?) ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, (R?) ======================================================================== HD 82210 24 UMA G4III-IV (EMISS H+K) AR 09 30.1 DEC +70 03 MV = 4.60 FE/H = - (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 82328 TET UMA F6IV AR 09 29.5 DEC +51 54 MV = 3.20 FE/H = 0 R ------------------------------------------------------------------------ (156) GREENSTEIN, J.L. 1948: ASTROPHYS.J. 107, 151 ........................................................................ OBSERV. : PG, 4010-4830A, 2.8 A/MM INSTRUM.: MCDONALD, COUDE LINELIST: LLWW, 350 ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3300-4700A, 9+13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T(BETA, R-I, B-V, B-Y, SCAN 5550-6750A) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 82885 11 LMI G8III VAR (EMISS H+K) AR 09 32.7 DEC +36 02 MV = 5.41 FE/H = 0 (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 83632 BD +26 1990 K2III AR 09 37.7 DEC +26 14 MV = 8.09 FE/H = --- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 83769 BD +01 2341 F5VI: (SUBDWARF) AR 09 38.2 DEC +01 15 MV = 10.23 FE/H = ---- (L) ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-5300A, 4.7 A/MM, 0.32 A INSTRUM.: CTIO 4M, ECHELLE, IT LINELIST: 25:, LLWW: CARNEY, PETERSON 1981: ASTROPHYS.J. 251, 190 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA, (L) ======================================================================== HD 84441 EPS LEO G1II AR 09 43.0 DEC +24 00 MV = 2.98 FE/H = 0 (R) ------------------------------------------------------------------------ ( 78) WILLIAMS, P.M. 1973: MONTHLY NOTICES ROY.ASTRON.SOC. 162, 235 ........................................................................ OBSERV. : PG, 4760-5150A, 2.2 A/MM INSTRUM.: RGO I.N.T., COUDE LINELIST: LW, 100: ANALYSIS: LTE(T-TAU SCALED FROM SUN), DIFF(SUN, EPS VIR), T(FE I, TI I EXCITATION; B-V,R-I, I-K), G(FE, TI IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 84737 15 LMI G0.5VA AR 09 45.4 DEC +46 15 MV = 5.10 FE/H = 0 (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 84810 L CAR G3IB AR 09 43.9 DEC -62 17 MV = 3.40 FE/H = 0 (R) ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5700-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON,; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 84903 CD -40 5513 GV:W (WEAK METALS) AR 09 45.3 DEC -41 13 MV = 7.9 FE/H = ---- R ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM (328) SPITE SPITE 1979: A+A 76, 150 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(R-I), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (328) SPITE, M., SPITE, F. 1979: ASTRON.ASTROPHYS. 76, 150 ........................................................................ OBSERV. : PG, 4320-4950A, 5130-6250A, 12 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LLWW, 240: ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(R-I, HBETA, HGAMMA), G(IONIZATION FE, TI, CR) REMARKS : TAKE INTO ACCOUNT VARIATION OF COG WITH EACH IONIC SPECIES: SOME IMPORTANCE FOR NA, MG, BA, Y COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (322) SPITE, M., SPITE, F. 1980: ASTRON.ASTROPHYS. 89, 118 ........................................................................ OBSERV. : PG, 3930-3970A, 7.1 A/MM INSTRUM.: ESO 1.5M, COUDE, ECHELLE, LALLEMAND EGC LINELIST: LW, 4 ANALYSIS: LTE(PEYTREMANN 1974, GUSTAFSSON), DIFF(SUN), T+G(SPITE'S 1979: A+A 76, 150), F-VALUES: WIESE 1969 NSRDS-NBS 22 SPECTRUM SYNTHESIS REMARKS : DERIVE AL ABUNDANCE ONLY COMMENTS: FE AND MG ABUNDANCES ARE QUOTED FROM OTHER WORKS CLASS : DMSA ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : DATA FROM (328) SPITE SPITE 1979: A+A 76, 150 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(SPITE), SOLAR F-VALUES REMARKS : REANALYSIS COMMENTS: CLASS : DMAA, R ======================================================================== HD 84937 BD +14 2151 F5VI (SUBDWARF, BLUE STRAGGLER) AR 09 46.2 DEC +13 59 MV = 8.28 FE/H = ---- R ------------------------------------------------------------------------ (244) GRABOWSKI, B. 1976: ACTA ASTRON. 26, 147 ........................................................................ OBSERV. : PG, 3600-4500A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG(WEIGHTING FUNCTIONS FROM LTE(CAYREL, JUGAKU) MODELS; COG SHAPE FROM SUN(COWLEY'S 1964: AP.J. 140, 713), UNSOELD 1968: STERNATMOSPHAEREN), DIFF(HD 140283, SUN), T(FE I EXCITATION; TI I/II IONIZATION, NE FROM BALMER LINES VIA INGLIS-TELLER FORMULA; HGAMMA PROFILE), F-VALUES: VARIOUS WORKS(1964-1975) AS LISTED REMARKS : COMMENTS: CLASS : DTMAA ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 120: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (300) PETERSON, R.C., CARNEY, B.W. 1979: ASTROPHYS.J. 231, 762 ........................................................................ OBSERV. : PG, 5170-5700A, 1.75 A/MM, 0.2 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 100: ANALYSIS: DIFF(SUN), LTE(ATLAS), T(R-I, V-K; SCAN 5000...8400 A), G(ASSUMED), F-VALUES(FE I): BRIDGES+KORNBLITH 1974, MAY ET AL.1974 DIFF(SUN) REMARKS : ANALYZE WEAK FE I LINES COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-4620A, 1.48 A/MM, 0.18 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 120:, LLWW: PETERSON 1978: ASTROPHYS.J. 222, 181 18:, LLWW: PETERSON, CARNEY 1979: ASTROPHYS.J. 231, 762 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL, CA, TI ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA, R ======================================================================== HD 85503 MU LEO K2III (EMISS H+K, CN) AR 09 49.9 DEC +26 15 MV = 3.88 FE/H = 0 R ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : PG, 4800-6300A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 220: ANALYSIS: DIFF(MEAN OF: GAM TAU, DEL TAU, EPS TAU, EPS VIR), LTE(ALTAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ ( 99) BLANC-VAZIAGA, M.-J., CAYREL , G., CAYREL, R. 1973: ASTROPHYS.J. 180, 871 ........................................................................ OBSERV. : PG, ??? , 12 A/MM, 0.28 A INSTRUM.: ESO 1.5M, COUDE; OHP 1.9M, COUDE, 2 A/MM, LALLEMAND EGC LINELIST: ANALYSIS: DIFF(EPS VIR), COG(T-TAU FROM LTE(PEYTREMANN 1970)), T+G(R-I, V-K; IONIZATION FE I/II, TI I/II, CR I/II; ABUNDANCE FROM WEAK AND STRONG LINES; ABSOLUTE MAG.) F-VALUES: DIFF(EPS VIR) REMARKS : ALSO COMPARE OBSERVED AND COMPUTED PROFILES OF NA I D, MG I B LINES COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 4.5+6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (217) PETERSON, R.C. 1976: ASTROPHYS.J.SUPPL. 30, 61 ........................................................................ OBSERV. : PG, 5190-5890A, 1.7 A/MM INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 200: ANALYSIS: LTE(EMPIRICAL), T(EXCITATION FE I, TI I), G(FE I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED, FE I: DIFF(SUN) REMARKS : COMMENTS: CLASS : (D)TGMAA, R ------------------------------------------------------------------------ (294) BRANCH, D., BONNELL, J., TOMKIN, J. 1978: ASTROPHYS.J. 225, 902 ........................................................................ OBSERV. : PE, RETICON, 7700-7870A, 8680-8780A, 0.12 A INSTRUM.: MCDONALD 2.7M, ECHELLE LINELIST: LW, 18 ANALYSIS: COG(THEOR.COG FROM LTE MODELS(GUSTAFSSON)), DIFF(SUN), T+G(LAMBERT, RIES 1977: AP.J. 217, 508) REMARKS : 30 LINES OF ELEMENTS OTHER THAN FE WERE ALSO MEASURED, BUT NOT FULLY ANALYZED COMMENTS: DERIVE FE ABUNDANCE ONLY CLASS : DMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R ======================================================================== HD 85504 7 SEX AOVS AR 09 49.6 DEC +02 41 MV = 6.02 FE/H = + (L) ------------------------------------------------------------------------ (141) WALLERSTEIN, G., STONE, Y.H., WILLIAMS, J.A. 1962: ASTROPHYS.J. 135, 459 ........................................................................ OBSERV. : PG, 3840-6500A, 10+15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 150: ANALYSIS: COG, DIFF(ALF CMA), T(FE I, FE II, TI II, SI II EXCITATION; UBV, G-I; SP.TYPE), ALSO: LTE(HUNGER 1955: Z.ASTROPHYS. 36, 42), F-VALUES: ALLEN 1955 REMARKS : COMMENTS: CLASS : DT(M)AA, (L) ======================================================================== HD 85773 BD -22 2754 K0 (WEAK METALS) AR 09 51.3 DEC -22 36 MV = 9.5 FE/H = ---- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-6800A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 86728 20 LMI G3VA AR 09 58.1 DEC +32 10 MV = 5.40 FE/H = 0 R ------------------------------------------------------------------------ ( 31) WALLERSTEIN, G., HELFER, H.L. 1961: ASTROPHYS.J. 133, 562 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 120:, LLWW: ( 29) HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE( IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, LLWW: HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 INSTRUM.: LINELIST: 15 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(PREVIOUS WORK....), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, R ------------------------------------------------------------------------ (A20) CORNIDE, M., REGO, M. 1984: ASTROPHYS.SPACE SCI. 105, 55 ........................................................................ OBSERV. : PG, 3900-5000A, 7.2 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: LW, 90 FE I LINES ANALYSIS: LTE(ATLAS), T(R-I, OTHER COLOURS), G(ABS.MAG.+RADIUS/COLOUR RELATION), T+G(TI I,II, FE I,II LINES), F-VALUES: FOY(1972)(DIFF(SUN)), BRIDGES+KORNBLITH) REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : DT(G)MA, L ======================================================================== HD 86986 BD +15 2156 A1V (HOR.BRANCH) AR 09 59.8 DEC +14 48 MV = 8.01 FE/H = --- R ------------------------------------------------------------------------ ( 72) KODAIRA, K., GREENSTEIN, J.L, OKE, J.B. 1969: ASTROPHYS.J. 155, 525 ........................................................................ OBSERV. : PG, 3900-4600A, 6 A/MM INSTRUM.: MT.PALOMAR 200-INCH LINELIST: LW, 80: ANALYSIS: COG, DIFF(HD 161817), THEOR.COG FROM WRUBEL(1949), T+G(HGAMMA, SCAN 4000-8000A, BJ; LTE MODELS(MIHALAS 1966)), F-VALUES: FE I: CORLISS BOZMAN(1962), FE II: RODER(1962) REMARKS : COMMENTS: CLASS : DTG(M)AA, L ------------------------------------------------------------------------ ( 69) KODAIRA, K. 1973: ASTRON.ASTROPHYS. 22, 273 ........................................................................ OBSERV. : DATA FROM ( 72) KODAIRA ET AL.1969: AP.J. 155, 425 INSTRUM.: LINELIST: ANALYSIS: ??? REMARKS : RE-ANALYZES DATA USING NEW F-VALUES COMMENTS: THIS IS MORE A SUMMARY OF RESULTS RATHER THAN A DETAILLED DESCRIPTION OF THE METHODS. THESE METHODS PROBABLY ARE THE SAME AS IN THE PREVIOUS STUDIES. CLASS : TAA, L? ------------------------------------------------------------------------ (379) DANFORD, S.C., LEA, S.M. 1981: ASTRON.J. 86, 1909 ........................................................................ OBSERV. : DATA FROM KODAIRA ET AL.1969: AP.J. 155, 525 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T+G(SCAN: DANFORD 1976: THESIS, YALE UNIV.) F-VALUES: VARIOUS SOURCES (1969-78) LISTED REMARKS : CONVERT EQU.WIDTHS TO SCALE OF WRIGHT ET AL.1964, REANALYSIS WITH IMPROVED DAMPING CONSTANTS COMMENTS: CLASS : MAA, R ======================================================================== HD 87737 ETA LEO A0IB AR 10 04.6 DEC +17 00 MV = 3.52 FE/H = 0 L ------------------------------------------------------------------------ (115) PRZYBYLSKI, A. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 146, 71 ........................................................................ OBSERV. : PG, 3670-6563A, 10.2+20.4 A/MM INSTRUM.: MT.STROMLO, COUDE LINELIST: LLWW, 550:, USED FOR ANALYSIS: 311 ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949) T+PE(FE IONIZATION) REMARKS : COMMENTS: CLASS : TAA, I ------------------------------------------------------------------------ (116) WOLF, B. 1971: ASTRON.ASTROPHYS. 10, 383 ........................................................................ OBSERV. : PG, 3150-4880A, 10+2.8 A/MM; 5875-6565A, 5.8+10 A/MM INSTRUM.: MT.WILSON 100-INCH, LICK LINELIST: LLWW, 560 ANALYSIS: LTE(UNBLANKETED; MIHALAS 1966), T+G(BJ; WIDTHS OF HGAMMA, HDELTA, H8; U-B; MG I/II), CHECKS: SCAN 3270-6050A; PROFILES OF HALFA, HBETA, HGAMMA, HDELTA; WIDTHS OF HALFA...H10, F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : ALSO GIVES RESULTS OF PRELIMINARY COG ANALYSIS COMMENTS: CLASS : TGMAA, L ======================================================================== HD 88218 HR3992 F8V AR 10 07.4 DEC -35 37 MV = 6.13 FE/H = - (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: OHP 1.5M, COUDE INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 88230 BD +50 1725 K8V (EMISS H+K) AR 10 08.3 DEC +49 42 MV = 6.61 FE/H = 0 (L) ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : PG, ???? , 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH LINELIST: 250 ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, (L) ======================================================================== HD 88284 LAM HYA K0III (EMISS H+K, CN) AR 10 08.1 DEC -12 06 MV = 3.61 FE/H = 0 R? ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 43) HELFER 1968: AP.J.SUPPL. 16, 1 INSTRUM.: LINELIST: ANALYSIS: DIFF(MEAN OF: GAM TAU, DEL TAU, EPS TAU, EPS VIR), LTE(ALTAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 88446 BD +18 2330 F8 AR 10 09.6 DEC +17 33 MV = 7.85 FE/H = - (R) ------------------------------------------------------------------------ (A30) LUCK, R.E., BOND, H.E. 1982: ASTROPHYS.J. 259, 792 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM; 50A SECTIONS IN 5100-7800A, 0.2A, S/N= 30..50 (RETICON) INSTRUM.: MT.WILSON 100-INCH, COUDE, RETICON LINELIST: 200 OR MORE ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 88609 BD +54 1359 G5IIIWE (WEAK METALS) AR 10 11.2 DEC +53 49 MV = 8.61 FE/H = ---- R ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O STELLAR PARAMATERS VERY UNCERTAIN TEMPERATURE LOWER THAN FROM SP.TYPE OR PHOTOMETRY COMMENTS: NO PHOTMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, R ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, V-K), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-6800A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 89010 35 LEO G1.5IV-V AR 10 13.8 DEC +23 45 MV = 5.90 FE/H = 0 (L) ------------------------------------------------------------------------ (324) CAYREL DE STROBEL, G., KNOWLES, N., HERNANDEZ, G., BENTOLILA, C. 1981: ASTRON.ASTROPHYS. 94, 1 ........................................................................ OBSERV. : PG, 4000-4900A, 12.4A/MM, 0.30A INSTRUM.: OHP 1.52M, COUDE LINELIST: LLWW, 210: ANALYSIS: COG, DIFF(SUN), T(B-Y, B2-V1, HBETA+HGAMMA), G(4383A) REMARKS : LOOKING FOR SOLAR TWINS COMMENTS: CLASS : DTGAA, (L) ======================================================================== HD 89125 39 LEO F8VBW AR 10 14.5 DEC +23 21 MV = 5.80 FE/H = 0 (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 89388 HR 4050 K3IIA (EMISS H+K) AR 10 15.6 DEC -61 05 MV = 3.40 FE/H = + R ------------------------------------------------------------------------ (177) HYLAND, A.R., MOULD, J.R. 1974: ASTROPHYS.J. 187, 277 ........................................................................ OBSERV. : PG, 5000-7000A, 1.5 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE, ECHELLE, IT LINELIST: LW, 7 ANALYSIS: BA/H: DIFF(HR 5058), COG FROM 30 FE I LINES, T(R-I) FE/H: COG(VAN DER HELD), DIFF(ALF BOO) REMARKS : DERIVE BA/H AND FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, I ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5300-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 89484 GAM1 LEO K1IIIB (EMISS H+K) AR 10 17.2 DEC +20 06 MV = 2.61 FE/H = - R? ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN SLIGHTLY WEAK COMMENTS: CLASS : (D)A ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6700A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 89485 GAM2 LEO G7IIICN... (EMISS H+K) AR 10 17.2 DEC +20 06 MV = 3.5 FE/H = + R? ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN SLIGHTLY WEAK COMMENTS: CLASS : (D)A ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6700A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 90508 HR 4098 F9V AR 10 25.0 DEC +49 03 MV = 6.44 FE/H = 0 I ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA, I ======================================================================== HD 90537 BET LMI G9III-IV (EMISS H+K) AR 10 25.0 DEC +36 58 MV = 4.21 FE/H = 0 (L) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (L) ======================================================================== HD 90839 36 UMA F8V AR 10 27.4 DEC +56 14 MV = 4.80 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 91324 HR 4134 F6V (WEAK METALS) AR 10 29.4 DEC -53 28 MV = 4.89 FE/H = -- (R) ------------------------------------------------------------------------ (191) DA SILVA, L. 1975: ASTRON.ASTROPHYS. 41, 287 ........................................................................ OBSERV. : PG, 4390-6600A, 3.2+12.4 A/MM, 0.14+0.30 A INSTRUM.: ESO 1.5M, COUDE LINELIST: DAOR, 400: ANALYSIS: LTE(PEYTREMANN 1970), DIFF(SUN), T(B-Y, R-I, BETA; WINGS OF HALFA, HBETA), T+G(PARALLAXES, MASS-LUMINOSITY REL.; IONIZATION FE, CR, TI), REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 93487 BD +24 2272 F8 AR 10 45.2 DEC +23 36 MV = 8.8 FE/H = --- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 5200-6800A, 2.3 A/MM, 0.1A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA ======================================================================== HD 94028 BD +21 2247 F4V (SUBDWARF, WEAK METALS) AR 10 48.8 DEC +20 33 MV = 8.23 FE/H = --- R ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : PG, 4500-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, EGC LINELIST: LLWW, 50: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (283) PETERSON, R.C. 1976: ASTROPHYS.J. 206, 800 ........................................................................ OBSERV. : PG, 3940-4760A, 1.5 A/MM INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), T(FE I EXCITATION), G(TI I/II IONIZATION), F-VALUES: FE I: BRIDGES, KORNBLITH 1974: AP.J. 192, 793 REMARKS : CHECK OF THE LABORATORY F-VALUES FOR FE I YIELDED A SIGNIFICANT DISAGREEMENT. COMMENTS: CLASS : TGMAA ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 120: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: CLASS : DTGMA ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM (283) PETERSON 1976: AP.J. 206, 800 INSTRUM.: LINELIST: USE LINES LONGWARD OF 4300 A ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(PETERSON), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : DATA FROM (245) HEARNSHAW 1976: A+A 51, 71 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION) REMARKS : REANALYSIS COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-4620A, 1.48 A/MM, 0.18 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 120:, LLWW: PETERSON 1978: ASTROPHYS.J. 222, 181 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL, CA, TI ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA, R ======================================================================== HD 94247 44 UMA K3III AR 10 50.5 DEC +54 51 MV = 5.10 FE/H = 0 (R) ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: OHP LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, (R) ======================================================================== HD 94264 46 LMI K0III (EMISS H+K) AR 10 50.5 DEC +34 29 MV = 3.83 FE/H = 0 L ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : PG, 4400-6800A, 9.7+12.4 A/MM, 0.3A INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(EPS VIR), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, L ======================================================================== HD 95128 47 UMA G1V AR 10 56.7 DEC +40 42 MV = 5.10 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 95272 ALF CRT K0III (EMISS H+K, CN) AR 10 57.3 DEC -18 02 MV = 4.07 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6700A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 95689 ALF UMA K0IAB: (EMISS H+K) AR 11 00.7 DEC +62 01 MV = 1.79 FE/H = 0 R? ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 95735 GJ 411 M2V (EMISS H+K) AR 11 00.6 DEC +36 18 MV = 7.49 FE/H = 0 (R) ------------------------------------------------------------------------ (313) MOULD, J.R., 1978: ASTROPHYS.J. 226, 923 ........................................................................ OBSERV. : 1.5-2.5 MU, 1.5 A (= 4000-6600CM**-1, 0.3 CM**-1) INSTRUM.: KPNO 4M, FTS LINELIST: LW, 22 ANALYSIS: LTE(MOULD 1976), SPECTRUM SYNTHESIS, T(7540-10175 COLOUR), F-VALUES: DIFF(SUN), THEORETICAL VALUES REMARKS : COMMENTS: CLASS : (D)TMSA, (R) ======================================================================== HD 96833 PSI UMA K1III (EMISS H+K) AR 11 06.9 DEC +44 46 MV = 3.00 FE/H = 0 R ------------------------------------------------------------------------ ( 49) YAMASHITA, Y., 1964: PUBL.DOM.ASTROPHYS.OBS.VICTORIA 12, 455 ........................................................................ OBSERV. : PG, 3700-6700A, 3.4-7 A/MM INSTRUM.: DAO 72-INCH, CASSEGRAIN LINELIST: LLWW, 800: ANALYSIS: COG, T(TI, V, FE, CO EXCITATION), F-VALUES: SOURCES AS LISTED (1938-1965) REMARKS : HYDROGEN ABUNDANCE IS DERIVED FROM CONTINUUM COMMENTS: CLASS : TAA ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 96918 HR 4337 G4... AR 11 06.4 DEC -58 42 MV = 3.90 FE/H = 0 (R) ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5700-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 97633 TET LEO A2V AR 11 11.6 DEC +15 42 MV = 3.34 FE/H = + L ------------------------------------------------------------------------ (133) KRIZ, S. 1966: BULL.ASTRON.INST.CZECH. 24, 71 ........................................................................ OBSERV. : PG, 3700-4860A, 1.3 A/MM INSTRUM.: CRIMEAN OBS. 2.6M, COUDE LINELIST: LLWW, 400: ANALYSIS: COG, THEOR.COG: HUNGER 1956: Z.ASTROPHYS. 39, 36 T(FE, TI, CR EXCITATION), F-VALUES: PRIV.COMM. 1965 REMARKS : COMMENTS: CLASS : TAA, I ------------------------------------------------------------------------ (124) SMITH, M.A. 1974: ASTROPHYS.J. 189, 101 ........................................................................ OBSERV. : PG, 3850-6170A, 8+16 A/MM INSTRUM.: LICK, COUDE LINELIST: LLWW, 260: ANALYSIS: LTE(ATLAS), T+G(SCHILD ET AL.1970: AP.J. 166, 95), REMARKS : AM STAR COMMENTS: CLASS : TMAA, L ======================================================================== HD 97907 73 LEO K3III AR 11 13.3 DEC +13 35 MV = 5.32 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 97916 BD +02 2406 F5V (WEAK METALS) AR 11 13.3 DEC +02 22 MV = 9.20 FE/H = --- R ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 120: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: CLASS : DTGMA ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-4620A, 1.48 A/MM, 0.18 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 120:, LLWW: PETERSON 1978: ASTROPHYS.J. 222, 181 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL, CA, TI ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA, R ======================================================================== HD 98430 DEL CRT G8III (EMISS H+K) AR 11 16.8 DEC -14 30 MV = 3.56 FE/H = - (R?) ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, (R?) ======================================================================== HD 99491 83 LEO K0IV AR 11 24.2 DEC +03 17 MV = 6.49 FE/H = 0 (R) ------------------------------------------------------------------------ (246) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 85 ........................................................................ OBSERV. : PG, EGC, 4650-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE LINELIST: LLWW, 200: ANALYSIS: LTE(PEYTREMANN 1974), DIFF(SUN), T(R-I), G(FE I/II IONIZ.) REMARKS : DERIVES FE ABUND. ONLY COMMENTS: CF. HEARNSHAW 1976: A.A. 51, 71 CLASS : DTGMA, (R) ======================================================================== HD 100006 86 LEO K0III AR 11 27.9 DEC +18 41 MV = 5.52 FE/H = 0 (R) ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: OHP LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, (R) ======================================================================== HD 100407 XI HYA G7III AR 11 30.5 DEC -31 35 MV = 3.54 FE/H = 0 (R) ------------------------------------------------------------------------ (288) COTTRELL, P.L., NORRIS, J. 1978: ASTROPHYS.J. 221, 893 ........................................................................ OBSERV. : PG, 5200-5500A, 1.5 A/MM; 4300-4325A, 1 A/MM, 0.4 A; 3883A REGION, 7 A/MM; 3360A REGION 10 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE, ECHELLE, IT, LINELIST: LW, 65 ANALYSIS: COG, DIFF(HD 28307), T(R-I) CN, CH, NH: SPECTRUM SYNTHESIS(ATLAS), LTE(GUSTAFSSON), F-VALUES: KURUCZ, PEYTREMANN 1975: SAO SPEC.REPT. 362 VARIED FROM VALUES OF OTHER AUTHORS, DIFF(SUN) REMARKS : COMMENTS: CLASS : DTMSA, (R) ======================================================================== HD 101501 61 UMA G8V (EMISS H+K) AR 11 38.4 DEC +34 29 MV = 3.22 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (A20) CORNIDE, M., REGO, M. 1984: ASTROPHYS.SPACE SCI. 105, 55 ........................................................................ OBSERV. : PG, 3900-5000A, 7.2 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: LW, 90 FE I LINES ANALYSIS: LTE(ATLAS), T(R-I, OTHER COLOURS), G(ABS.MAG.+RADIUS/COLOUR RELATION), T+G(TI I,II, FE I,II LINES), F-VALUES: FOY(1972)(DIFF(SUN)), BRIDGES+KORNBLITH) REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : DT(G)MA, L ======================================================================== HD 102212 NU VIR M1III (EMISS H+K) AR 11 43.3 DEC +06 49 MV = 4.03 FE/H = - (R) ------------------------------------------------------------------------ (A10) SMITH, V.V., LAMBERT, D.L. 1985: ASTROPHYS.J. 294, 326 ........................................................................ OBSERV. : PE, REGIONS BETWEEN 7330-7600 A, 0.2 A (RETICON) 1.6 + 2.2 MICRON (4500 CM**-1), 0.05 CM**-1 (FTS) INSTRUM.: MCDONALD 2.7M, COUDE, RETICON; KPNO 4M, FTS LINELIST: LW, 29 ATOMIC + 60 MOLECULAR LINES ANALYSIS: LTE(JOHNSON), DIFF(ALF TAU), T(V-K), G(ABS.MAG.+EVOL.TRACKS) F-VALUES: CF. LAMBERT ET AL. 1984: AP.J. 284, 223 REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 102224 KHI UMA K0.5IIIB (EMISS H+K+MG(UV)) AR 11 43.4 DEC +48 03 MV = 3.71 FE/H = -- (L) ------------------------------------------------------------------------ ( 49) YAMASHITA, Y., 1964: PUBL.DOM.ASTROPHYS.OBS.VICTORIA 12, 455 ........................................................................ OBSERV. : PG, 3700-6700A, 3.4-7 A/MM INSTRUM.: DAO 72-INCH, CASSEGRAIN LINELIST: LLWW, 800: ANALYSIS: COG, DIFF(PSI UMA), T(TI, V, FE, CO EXCITATION), F-VALUES: SOURCES AS LISTED (1938-1965) REMARKS : HYDROGEN ABUNDANCE IS DERIVED FROM CONTINUUM COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 102365 HR4523 G5V AR 11 44.1 DEC -40 14 MV = 4.89 FE/H = -- R ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (287) KOVACS, N., FOY, R. 1978: ASTRON.ASTROPHYS. 68, 27 ........................................................................ OBSERV. : DATA FROM ( 86) HEARNSHAW 1972: MEM.RAS 77, 55 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM MODELS LTE(PEYTREMANN 1974)), DIFF(SUN), T(R-I), G(IONIZATION FE I/II), F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: GIVE FE/H RATIO ONLY CLASS : DTGMAA, R ======================================================================== HD 102634 HR 4533 F7V AR 11 46.5 DEC -00 02 MV = 6.15 FE/H = 0 L ------------------------------------------------------------------------ ( 50) CAYREL DE STROBEL, G. 1968: ANN.ASTROPHYS. 31, 43 ........................................................................ OBSERV. : PG, 3940-4650A, 4.5+8.9 A/MM, 0.14+0.18 A INSTRUM.: MT.PALOMAR 200-INCH, KPNO, COUDE LINELIST: LLWW, 300: ANALYSIS: COG, DIFF(SUN), T(B-Y: LTE(CAYREL, JUGAKU)), G(IONIZATION) REMARKS : COMMENTS: CLASS : DTG(M)AA, L ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : DATA: ( 50) CAYREL DE STROBEL 1968: ANN.ASTROPHYS. 31, 43 INSTRUM.: LINELIST: 12 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(PREVIOUS WORK.....), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ======================================================================== HD 102870 BET VIR F8V AR 11 48.1 DEC +02 03 MV = 3.61 FE/H = 0 R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA, L ------------------------------------------------------------------------ ( 59) BASCHEK, B., HOLWEGER, H., NAMBA, O., TRAVING, G. 1967: Z.ASTROPHYS. 65, 418 ........................................................................ OBSERV. : PG, 4200-6800A, 4.5+10+15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 520: ANALYSIS: DIFF(SUN), LTE(SCALED EMPIRICAL SOLAR MODEL BY HOLWEGER 1967: Z.ASTROPHYS. 65, 365) T(SCAN 3390-5560A; BJ; UBVIJK, UVBGRI; PROFILES OF HBETA, HGAMMA; LINE EXCITATION), G(TRIG.PARALL.+ABS.MAG., IONIZATION EQ.) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : DATA FROM ( 59) BASCHEK ET AL.1967: Z.ASTROPHYS. 65, 418 INSTRUM.: LINELIST: 43 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE M0DELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ------------------------------------------------------------------------ (316) GEHREN, T. 1978: ASTRON.ASTROPHYS. 65, 427 ........................................................................ OBSERV. : DATA FROM ( 59) BASCHEK ET AL.1967: Z.ASTROPHYS. 65, 418 PLUS: PG, REGION AT 7770A, 10+20 A/MM INSTRUM.: MT.STROMLO 74-INCH, IT LINELIST: LW, 3 ANALYSIS: DIFF(SUN), LTE(SCALED EMPIRICAL SOLAR MODEL FROM HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19) T(PROFILES OF HBETA, HGAMMA), G(SI, TI, CR, FE IONIZATION), F-VALUES: DIFF(SUN) REMARKS : ABSOLUTE MAGNITUDE, COLOURS, AND SCANS ARE FOUND TO BE FITTED REASONABLY WELL BY THE MODEL, BUT WERE NOT USED TO DERIVE THE STELLAR PARAMETERS. COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (316) GEHREN 1978: A+A 65, 427 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 103036 TY VIR G3IBPVAR (WEAK METALS) AR 11 49.3 DEC -05 29 MV = 8.00 FE/H = --- R ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 6.8 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE, IT LINELIST: 50 ANALYSIS: DIFF(SUN, EPS VIR), COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 5200-6800A, 2.3 A/MM, 0.1A INSTRUM.: KPNO 4M, CTIO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 103095 GMB 1830 G8VP (SUBDWARF, EMISS H+K) AR 11 50.1 DEC +38 05 MV = 6.45 FE/H = --- R ------------------------------------------------------------------------ ( 96) TOMKIN, J. 1972: MONTHLY NOTICES ROY.ASTRON.SOC. 156, 349 ........................................................................ OBSERV. : PG, 3770-4640A, 2.8+4.5 A/MM; 5580-6170,6300-6580A, 6.8 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: 180:, LLWW: TOMKIN 1972?: TO BE PUBLISHED ANALYSIS: COG, DIFF(SUN), T(FE I COG, AGREES WITH UBV, GRI, R-I, V-K) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (306) TOMKIN, J., BELL, R.A. 1973: MONTHLY NOTICES ROY.ASTRON.SOC. 163, 117 ........................................................................ OBSERV. : DATA FROM ( 96) TOMKIN 1972: MNRAS 156, 349 PLUS: PG, REGIONS AT 3870A (CN), 4220A (CH), 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, LINELIST: ANALYSIS: LTE(T-TAU SCALED FROM SUN(HSRA)), T(FE I COG, R-I, 6-COLOUR PHOTM.), G(ABSOLUTE MAG.), T(CHECKED WITH SCAN 3700-6550A), F-VALUES: VARIOUS SOURCES AS GIVEN REMARKS : REVISE FE, C, N ABUNDANCES OF ( 96) TOMKIN 1972 COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : PG, 4500-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, EGC LINELIST: LLWW, 150: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (260) CAYREL, G., CAYREL, R., FOY, R. 1977: ASTRON.ASTROPHYS. 54, 797 ........................................................................ OBSERV. : DATA FROM ( 96) TOMKIN 1972, AND OTHER SOURCES INSTRUM.: LINELIST: L, 200 SOLAR F-VALUES (FE I, II; 4510-6800A) ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1970) MODELS), T(VRIK, G-I), G(IONIZATION), T+G(CHECKED WITH NA I D, MG IB LINE PROFILES, ABS.MAG.), F-VALUES: DIFF(SUN) REMARKS : STUDY THE SPLITTING IN THE DAMPING PART OF THE FE COG COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (300) PETERSON, R.C., CARNEY, B.W. 1979: ASTROPHYS.J. 231, 762 ........................................................................ OBSERV. : PG, 5170-5700A, 1.75 A/MM, 0.2 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 100: ANALYSIS: DIFF(SUN), LTE(ATLAS), T(R-I, V-K; SCAN 5000...8400 A), G(ASSUMED), F-VALUES(FE I): BRIDGES+KORNBLITH 1974, MAY ET AL.1974 DIFF(SUN) REMARKS : ANALYZE WEAK FE I LINES COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : PG, 4485-5615A, 13 A/MM, 0.3 A INSTRUM.: OHP 1.5M, ECHELLE, EGC LINELIST: LLWW, 80: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION), F-VALUES: FOY (1972) REMARKS : ALSO REANALYZE DATA OF (245) HEARNSHAW 1976: A+A 51, 71 HEARNSHAW'S MEASUREMENTS OF WEAKEST LINES MAY HAVE BEEN OVERESTIMATED, COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : PG, PORTIONS IN THE RANGE 4600-6600A, 0.28 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: LLWW, LESS THAN 150: ANALYSIS: LTE(ATLAS), T(R-I, V-K), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVES FE/H ONLY, INCLUDES STRONGER LINES EXCLUDED BY (300) PETERSON, CARNEY 1979: AP.J. 231, 762 COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (312) TOMKIN, J., LAMBERT, D.L., 1980: ASTROPHYS.J. 235, 925 ........................................................................ OBSERV. : PE, RETICON, 20A SECTIONS AT 5140, 6160, 6320, 6700A 0.08A, S/N=100 INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE LINELIST: LW, 17 ANALYSIS: LTE(GUSTAFSSON), T(R-I, SCANS) REMARKS : DERIVE ABUNDANCES OF MG ISOTOPES FROM MGH BAND LINES, AND NA, MG, AL, CA, V, FE ATOMIC ABUND. COMMENTS: CLASS : (T)MA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 5170-5700A, 1.91 A/MM, 0.22 A (SAO), 5250-6680A, 5.5 A/MM, 0.29 A (KPNO) INSTRUM.: SAO 1.5M, ECHELLE, EGC; KPNO 4M, ECHELLE, IT LINELIST: 140:, LLWW: PETERSON, CARNEY 1979: ASTROPHYS.J. 231, 762 150:, LLWW: PETERSON 1979: ASTROPHYS.J. 235, 491 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 103578 95 LEO A3V AR 11 53.1 DEC +15 51 MV = 5.50 FE/H = 0 I ------------------------------------------------------------------------ ( 11) CHAMBERLAIN, J.W., ALLER, L.H. 1951: ASTROPHYS.J. 114, 52 ........................................................................ OBSERV. : PG, 4064-4732A, 10 A/MM, HGAMMA WITH 20 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE, ANN ARBOR 37-INCH LINELIST: LLWW, 65: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66), LTE MODELS, F-VALUES: KING 1938+42, T+G(FE I/II IONIZATION, PROFILES OF HBETA, HGAMMA, HDELTA, AND CA I K LINES) REMARKS : DERIVE FE AND CA ABUNDANCES COMMENTS: CLASS : TG(M)A, I ------------------------------------------------------------------------ (374) WOLFF, S.C. 1970: ASTROPHYS.J.SUPPL. 15, 21 ........................................................................ OBSERV. : PG, 3860-4620A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LW, 22 SELECTED UNBLENDED LINES ANALYSIS: COG(WRUBEL 1949), T(SCAN 4000-8800A, LTE(MIHALAS 1966)), G(HGAMMA PROFILES, LTE(MIHALAS 1966)), F-VALUES: WARNER 1967, CORLISS, BOZMAN 1962 REMARKS : USES ONLY ONE OR TWO LINES PER ION, MOST OF WHICH LIE ON THE COG'S FLAT PORTION. COMMENTS: THIS STAR SERVES AS STANDARD FOR STUDY OF AP STARS CLASS : TG(M)A, I ======================================================================== HD 104304 HR4587 G9IV AR 11 58.2 DEC -10 10 MV = 5.54 FE/H = 0 (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 104893 CD -28 4390 K0 (WEAK METALS) AR 12 02.1 DEC -28 54 MV = 9.5 FE/H = --- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-6800A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 105452 ALF CRV F2III-IV AR 12 05.8 DEC -24 27 MV = 4.00 FE/H = -- (R) ------------------------------------------------------------------------ (191) DA SILVA, L. 1975: ASTRON.ASTROPHYS. 41, 287 ........................................................................ OBSERV. : PG, 4390-6600A, 3.2+12.4 A/MM, 0.14+0.30 A INSTRUM.: ESO 1.5M, COUDE LINELIST: DAOR, 270: ANALYSIS: LTE(PEYTREMANN 1970), DIFF(SUN), T(B-Y, R-I, BETA; WINGS OF HALFA, HBETA), T+G(PARALLAXES, MASS-LUMINOSITY REL., IONIZATION FE, CR, TI) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 105546 BD +59 4122 G2IIIM (WEAK METALS) AR 12 06.5 DEC +59 18 MV = 8.61 FE/H = --- R ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3300-3700A, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, KPNO 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, R ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, V-K), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 105590 BD -11 3246 G0 AR 12 06.9 DEC -11 35 MV = 6.56 FE/H = 0 (R) ------------------------------------------------------------------------ ( 90) ZIELKE, G. 1970: ASTRON.ASTROPHYS. 6, 206 ........................................................................ OBSERV. : PG, 3900-4800A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LESS THAN 600:, LLWW: ZIELKE 1970: A+A SUPPL. 2, 205 ANALYSIS: LTE(T-TAU SCALED FROM SUN: HOLWEGER 1967: Z.AP. 65, 365), DIFF(HD 136202), T(PROFILES OF HALFA, HBETA, HGAMMA, HDELTA; BVGRI; LINE EXCITATION), G(IONIZATION SI, SC, TI, V, CR, FE, SR), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 105755 BD +55 1514 G0VM (WEAK METALS) AR 12 07.8 DEC +54 46 MV = 8.59 FE/H = --- (R) ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3300-3700A, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, KPNO 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, (R) ======================================================================== HD 106038 BD +14 2481 F6V-VI (SUBDWARF) AR 12 09.5 DEC +13 33 MV = 10.18 FE/H = --- (L) ------------------------------------------------------------------------ (244) GRABOWSKI, B. 1976: ACTA ASTRON. 26, 147 ........................................................................ OBSERV. : PG, 3600-4500A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG(WEIGHTING FUNCTIONS FROM LTE(CAYREL, JUGAKU) MODELS; COG SHAPE FROM SUN(COWLEY'S 1964: AP.J. 140, 713), UNSOELD 1968: STERNATMOSPHAEREN), DIFF(HD 140283, SUN), T(FE I EXCITATION; TI I/II IONIZATION, NE FROM BALMER LINES VIA INGLIS-TELLER FORMULA; HGAMMA PROFILE), F-VALUES: VARIOUS WORKS(1964-1975) AS LISTED REMARKS : COMMENTS: CLASS : DTMAA, (L) ======================================================================== HD 106304 CD -40 7168 B9V AR 12 11.3 DEC -40 36 MV = 9.08 FE/H = ? (L) ------------------------------------------------------------------------ (201) PRZYBYLSKI, A., 1971: MONTHLY NOTICES ROY.ASTRON.SOC. 153, 111 ........................................................................ OBSERV. : PG, ??? , 10.2 A/MM INSTRUM.: MT.STROMLO, COUDE LINELIST: 150 ANALYSIS: COG, DIFF(ALF LYR), THEOR.COG WRUBEL 1949: AP.J. 109, 66 T(UBV, SCAN), PE(INGLIS-TELLER; BJ, BALMER LINE WIDTHS; IONIZATION), REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 106516 HR 4657 F5V (WEAK METALS) AR 12 12.6 DEC -10 01 MV = 6.57 FE/H = -- R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 50) CAYREL DE STROBEL, G. 1968: ANN.ASTROPHYS. 31, 43 ........................................................................ OBSERV. : PG, 3940-4650A, 4.5+8.9 A/MM, 0.14+0.18 A INSTRUM.: MT.PALOMAR 200-INCH, KPNO, COUDE LINELIST: LLWW, 300: ANALYSIS: COG, DIFF(SUN), T(B-Y: LTE(CAYREL, JUGAKU)), G(IONIZATION) REMARKS : COMMENTS: CLASS : DTG(M)AA, L ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 120: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) F-VALUES: DIFF(SUN, DISK-CENTRE), EXPERIM.(ARC) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: CLASS : DTGMA ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : PG, PORTIONS IN THE RANGE 4600-6600A, 0.28 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: LLWW, LESS THAN 150: ANALYSIS: LTE(ATLAS), T(R-I, V-K), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM.(FURNACE) REMARKS : DERIVES FE/H ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-4620A, 1.48 A/MM, 0.18 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 120:, LLWW: PETERSON 1978: ASTROPHYS.J. 222, 181 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL, CA, TI ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 107213 9 COM F8VS AR 12 17.0 DEC +28 26 MV = 6.33 FE/H = 0 R ------------------------------------------------------------------------ (317) GEHREN, T. 1979: ASTRON.ASTROPHYS. 75, 73 ........................................................................ OBSERV. : PG, 4400-6820A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 480:, LLWW: GEHREN ET AL.1978: A+A SUPPL. 31, 297 ANALYSIS: LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), T(LINE PROFILES OF HALFA, HGAMMA), G(IONIZATION SI, TI, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (317) GEHREN 1979: A+A 75, 73 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 107259 ETA VIR A2IV AR 12 17.4 DEC -00 23 MV = 3.89 FE/H = 0 (I) ------------------------------------------------------------------------ (374) WOLFF, S.C. 1970: ASTROPHYS.J.SUPPL. 15, 21 ........................................................................ OBSERV. : PG, 3860-4620A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LW, 22 SELECTED UNBLENDED LINES ANALYSIS: COG(WRUBEL 1949), T(SCAN 4000-8800A, LTE(MIHALAS 1966)), G(HGAMMA PROFILES, LTE(MIHALAS 1966)), F-VALUES: WARNER 1967, CORLISS, BOZMAN 1962 REMARKS : USES ONLY ONE OR TWO LINES PER ION, MOST OF WHICH LIE ON THE COG'S FLAT PORTION. COMMENTS: THIS STAR SERVES AS STANDARD FOR STUDY OF AP STARS CLASS : TG(M)A, (I) ======================================================================== HD 107328 16 VIR K0IIIB (EMISS H+K) AR 12 17.8 DEC +03 35 MV = 5.00 FE/H = - L ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, L ======================================================================== HD 107369 CD -31 9638 A2II/III AR 12 18.1 DEC -32 17 MV = 9.5 FE/H = 0 R ------------------------------------------------------------------------ (405) KODAIRA, K., PHILIP, A.G.D. 1981: ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS, IAU COLLOQ. NO.68, A.G.D.PHILIP, D.S.HAYES EDS., L.DAVIS PRESS, SCHENECTADY, N.Y., P. 153 ........................................................................ OBSERV. : ??? 12.5 A/MM ?? INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: ANALYSIS: LTE(ATLAS), T+G(PHOTOMETRY, HDELTA PROFILE) REMARKS : GIVE FE/H ONLY COMMENTS: SUPERSEDED BY (A22) CLASS : TGMA ------------------------------------------------------------------------ (A22) KODAIRA, K., PHILIP, A.G.D. 1984: ASTROPHYS.J. 278, 208 ........................................................................ OBSERV. : PG, 3850-4300A, 12.5 A/MM INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), DIFF(HD 161817), T+G(B-V, C1, M1, HDELTA WING), F-VALUES: KURUCZ+PEYTREMANN 1975 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 107752 BD +12 2458 G5 (WEAK METALS) AR 12 20.3 DEC +11 52 MV = 10.0 FE/H = ---- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 108177 BD +02 2538 F5VI (SUBDWARF) AR 12 23.0 DEC +01 34 MV = 9.66 FE/H = --- R ------------------------------------------------------------------------ (244) GRABOWSKI, B. 1976: ACTA ASTRON. 26, 147 ........................................................................ OBSERV. : PG, 3600-4500A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG(WEIGHTING FUNCTIONS FROM LTE(CAYREL, JUGAKU) MODELS; COG SHAPE FROM SUN(COWLEY'S 1964: AP.J. 140, 713), UNSOELD 1968: STERNATMOSPHAEREN), DIFF(HD 140283, SUN), T(FE I EXCITATION; TI I/II IONIZATION, NE FROM BALMER LINES VIA INGLIS-TELLER FORMULA; HGAMMA PROFILE), F-VALUES: VARIOUS WORKS(1964-1975) AS LISTED REMARKS : COMMENTS: CLASS : DTMAA ------------------------------------------------------------------------ (283) PETERSON, R.C. 1976: ASTROPHYS.J. 206, 800 ........................................................................ OBSERV. : PG, 3940-4760A, 1.5 A/MM INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), T(FE I EXCITATION), G(TI I/II IONIZATION), F-VALUES: FE I: BRIDGES, KORNBLITH 1974: AP.J. 192, 793 REMARKS : CHECK OF THE LABORATORY F-VALUES FOR FE I YIELDED A SIGNIFICANT DISAGREEMENT. COMMENTS: CLASS : TGMAA ------------------------------------------------------------------------ (279) PETERSON, R.C. 1978: ASTROPHYS.J. 222, 181 ........................................................................ OBSERV. : PG, 3900-4620A, 1.5 A/MM, 0.17 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: LLWW, 120: ANALYSIS: LTE(ATLAS), T(R-I), G(IONIZATION), F-VALUES DIFF(SUN) REMARKS : GIVES FE/H RATIO ONLY COMMENTS: CLASS : DTGMA ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM (283) PETERSON 1976: AP.J. 206, 800 INSTRUM.: LINELIST: USE LINES LONGWARD OF 4300 A ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(PETERSON), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : DATA FROM (279) PETERSON 1978: AP.J. 222, 181 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I, V-K, SCAN 5000-8400A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, INTEGR.FLUX), EXPERIM. BLACKWELL ET AL.1979: MNRAS 186, 657 REMARKS : DERIVES FE/H ONLY COMMENTS: RE-ANALYSIS WITH REVISED T+G, MICROTURB., F-VALUES CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 3900-4620A, 1.48 A/MM, 0.18 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 120:, LLWW: PETERSON 1978: ASTROPHYS.J. 222, 181 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL, CA, TI ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 108317 BD +06 2613 G0 (WEAK METALS) AR 12 24.0 DEC +05 35 MV = 8.3 FE/H = ---- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 108381 GAM COM K1III (CN, EMISS H+K) AR 12 24.4 DEC +28 33 MV = 4.36 FE/H = 0 (L) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (L) ======================================================================== HD 109358 BET CVN G0V AR 12 31.4 DEC +41 38 MV = 4.26 FE/H = 0 R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (317) GEHREN, T. 1979: ASTRON.ASTROPHYS. 75, 73 ........................................................................ OBSERV. : PG, 4400-6820A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 480:, LLWW: GEHREN ET AL.1978: A+A SUPPL. 31, 297 ANALYSIS: LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), T(LINE PROFILES OF HALFA, HBETA), G(IONIZATION SI, TI, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (317) GEHREN 1979: A+A 75, 73 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ------------------------------------------------------------------------ (A20) CORNIDE, M., REGO, M. 1984: ASTROPHYS.SPACE SCI. 105, 55 ........................................................................ OBSERV. : PG, 3900-5000A, 7.2 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: LW, 90 FE I LINES ANALYSIS: LTE(ATLAS), T(R-I, OTHER COLOURS), G(ABS.MAG.+RADIUS/COLOUR RELATION), T+G(TI I,II, FE I,II LINES), F-VALUES: FOY(1972)(DIFF(SUN)), BRIDGES+KORNBLITH) REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : DT(G)MA, L ======================================================================== HD 109995 BD +40 25558 A0VP (HOR.BRANCH) AR 12 36.4 DEC +39 35 MV = 7.62 FE/H = - R ------------------------------------------------------------------------ ( 36) WALLERSTEIN, G., HUNZIGER, W. 1964: ASTROPHYS.J. 140, 214 ........................................................................ OBSERV. : PG, 3800-4800A, 4.4+10 A/MM; 5000-6600A, 16 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE ; LICK? 120-INCH, COUDE LINELIST: LW, 75: ANALYSIS: COG, DIFF(ALF CMA, ALF LYR), T(B-I) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 72) KODAIRA, K., GREENSTEIN, J.L, OKE, J.B. 1969: ASTROPHYS.J. 155, 525 ........................................................................ OBSERV. : PG, 3900-4600A, 6 A/MM INSTRUM.: MT.PALOMAR 200-INCH LINELIST: LW, 80: ANALYSIS: COG, DIFF(HD 161817), THEOR.COG FROM WRUBEL(1949), T+G(HGAMMA, SCAN 4000-8000A, BJ; LTE MODELS(MIHALAS 1966)), F-VALUES: FE I: CORLISS BOZMAN(1962), FE II: RODER(1962) REMARKS : COMMENTS: CLASS : DTG(M)AA, L ------------------------------------------------------------------------ ( 69) KODAIRA, K. 1973: ASTRON.ASTROPHYS. 22, 273 ........................................................................ OBSERV. : DATA FROM ( 72) KODAIRA ET AL.1969: AP.J. 155, 525 INSTRUM.: LINELIST: ANALYSIS: ??? REMARKS : RE-ANALYZES DATA USING NEW F-VALUES COMMENTS: THIS IS MORE A SUMMARY OF RESULTS RATHER THAN A DETAILLED DESCRIPTION OF THE METHODS. THESE METHODS PROBABLY ARE THE SAME AS IN THE PREVIOUS STUDIES. CLASS : TAA, L? ------------------------------------------------------------------------ (379) DANFORD, S.C., LEA, S.M. 1981: ASTRON.J. 86, 1909 ........................................................................ OBSERV. : DATA FROM ( 72) KODAIRA ET AL.1969: AP.J. 155, 525 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T+G(CONT: DANFORD 1976: THESIS, YALE UNIV.) F-VALUES: VARIOUS SOURCES (1969-78) LISTED REMARKS : CONVERT EQU.WIDTHS TO SCALE OF WRIGHT ET AL.1964, REANALYSIS WITH IMPROVED DAMPING CONSTANTS COMMENTS: CLASS : MAA, R ======================================================================== HD 110184 BD +09 2653 G5 (WEAK METALS) AR 12 37.7 DEC +08 48 MV = 8.27 FE/H = ---- R ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 6.8 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE, IT; KPNO 4M, ECHELLE LINELIST: 150 ANALYSIS: DIFF(SUN, EPS VIR), COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, V-K, B-V), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-6800A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, TO BE PUBL. SEPARATELY ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A15) SNEDEN, C., PILACHOWSKI, C.A. 1985: ASTROPHYS.J. 288, L55 ........................................................................ OBSERV. : PE, 9 RANGES IN 4100-6500A, 0.17 A, S/N= 40..100 INSTRUM.: KPNO 4M, CASSEGRAIN, ECHELLE, CCD LINELIST: 174 ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563), T+G(SNEDEN, PARTHASARATHY 1983: AP.J. 267, 757) REMARKS : COMMENTS: CLASS : DMAA ======================================================================== HD 110379 GAM VIR F0V AR 12 39.1 DEC -01 11 MV = 3.65 FE/H = -- (R?) ------------------------------------------------------------------------ (123) SMITH, M.A. 1971: ASTRON.ASTROPHYS. 11, 325 ........................................................................ OBSERV. : PG, ???? , 8.9+17.8 A/MM INSTRUM.: KPNO 84-INCH, COUDE LINELIST: LW: SMITH 19??: A+A SUPPL. ????????? ANALYSIS: LTE(ATLAS), T+G(FE I/II LINES), REMARKS : COMMENTS: CLASS : TGMAA, (R?) ======================================================================== HD 110897 10 CVN G0V AR 12 42.6 DEC +39 33 MV = 6.00 FE/H = - R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 111631 BD +00 2989 MV... AR 12 48.2 DEC -00 29 MV = 8.48 FE/H = 0 (L) ------------------------------------------------------------------------ (255) HARTMANN, L., ANDERSON, C.M. 1977: ASTROPHYS.J. 215, 177 ........................................................................ OBSERV. : PG, 5900-6600A, 0.1 A INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: ANALYSIS: COG(SOLAR FE I COG(FOY 1972: A+A 18, 26), SHIFTS FROM LTE(CARBON, GINGERICH) MODELS), DIFF(SUN, HSRA), T(V-K, R-I), G(ASSUMED), T+G CHECKED WITH FE, TI, V, CA IONIZATION REMARKS : ALSO USE MODELS OF JOHNSON 1974: NCAR TECH.NOTE, STR-95 COMMENTS: CLASS : DTMAA, (L) ======================================================================== HD 112033 35 COM G8III+... (EMISS H+K) AR 12 50.8 DEC +21 31 MV = 4.90 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 112127 BD +27 2189 K2.5III (CN) AR 12 51.5 DEC +27 03 MV = 6.91 FE/H = 0 R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 16.3 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (383) WALLERSTEIN, G., SNEDEN, C. 1982: ASTROPHYS.J. 255, 577 ........................................................................ OBSERV. : PG, 6540-6775A, 10 A/MM (DAO); RETICON, 100A RANGES AT 5050, 6100, 6720, 6710, 8020, 8120A 0.21-0.33 A, S/N= 150-260 (MCDONALD) INSTRUM.: DAO 1.2M, COUDE; MCDONALD 2.1M+2.7M, COUDE LINELIST: 60: ANALYSIS: LTE(GUSTAFSSON), DIFF(EPS VIR, SUN) T(SCAN 5000-10000A), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN)??? REMARKS : USE HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19 MODEL FOR THE SUN COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 112300 DEL VIR M3III (EMISS H+K) AR 12 53.1 DEC +03 40 MV = 3.38 FE/H = 0 (R) ------------------------------------------------------------------------ (A10) SMITH, V.V., LAMBERT, D.L. 1985: ASTROPHYS.J. 294, 326 ........................................................................ OBSERV. : PE, REGIONS BETWEEN 7330-7600 A, 0.2 A (RETICON) 1.6 + 2.2 MICRON (4500 CM**-1), 0.05 CM**-1 (FTS) INSTRUM.: MCDONALD 2.7M, COUDE, RETICON; KPNO 4M, FTS LINELIST: LW, 29 ATOMIC + 60 MOLECULAR LINES ANALYSIS: LTE(JOHNSON), DIFF(ALF TAU), T(V-K), G(ABS.MAG.+EVOL.TRACKS) F-VALUES: CF. LAMBERT ET AL. 1984: AP.J. 284, 223 REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 112989 37 COM G9III (EMISS H+K) AR 12 57.9 DEC +31 03 MV = 4.90 FE/H = 0 R? ------------------------------------------------------------------------ ( 49) YAMASHITA, Y., 1964: PUBL.DOM.ASTROPHYS.OBS.VICTORIA 12, 455 ........................................................................ OBSERV. : PG, 3700-6700A, 3.4-7 A/MM INSTRUM.: DAO 72-INCH, CASSEGRAIN LINELIST: LLWW, 800: ANALYSIS: COG, DIFF(PSI UMA, CHI UMA), T(TI, V, FE, CO EXCITATION), F-VALUES: SOURCES AS LISTED (1938-1965) REMARKS : HYDROGEN ABUNDANCE IS DERIVED FROM CONTINUUM COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 113226 EPS VIR G8III (EMISS H+K+MG(UV)) AR 12 59.7 DEC +11 14 MV = 2.83 FE/H = 0 R ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : COMMENTS: CLASS : (D)A ------------------------------------------------------------------------ ( 4) CAYREL, G., CAYREL, R. 1963: ASTROPHYS.J. 137, 431 ........................................................................ OBSERV. : PG, 4500-6700A, 1+2.8 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 1400 ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS(T-TAU RELATION FROM SEMIEMPIRICAL SOLAR MODEL), T(B-V, FE I EXCITATION, HALFA WINGS), G(DENSITY FROM COLL.DAMPING OF MG I LINE WINGS) REMARKS : ALSO CONSIDER MODELS WITH SOLAR T-TAU RELATION USED BY GOLDBERG AT AL.1960: AP.J. SUPPL. 5, 1 COMMENTS: CLASS : DTGMAA ------------------------------------------------------------------------ ( 6) HELFER, H.L., WALLERSTEIN, G. 1964: ASTROPHYS.J.SUPPL. 9, 81 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL'S 1963: AP.J. 137, 431 INSTRUM.: LINELIST: ANALYSIS: COG(AVERAGED EMPIRICAL COG FROM FE I), DIFF(AVERAGE OF: GAM TAU, DEL TAU, EPS TAU), T(FE I EXCITATION) REMARKS : COMMENTS: PAPER MAINLY CONCERNED WITH DERIVING ABUNDANCES RELATIVE TO FE IN THE 3 HYADES GIANTS, RELATIVE TO THE SUN CLASS : DTA ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL, CAYREL 1963: AP.J. 137, 431 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : RE-ANALYIS COMMENTS: CLASS : DTGMAA ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN ??? INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY ??? DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL 1963: AP.J. 137, 431 INSTRUM.: LINELIST: ANALYSIS: DIFF(SUN), LTE(ATLAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA ------------------------------------------------------------------------ ( 99) BLANC-VAZIAGA, M.-J., CAYREL , G., CAYREL, R. 1973: ASTROPHYS.J. 180, 871 ........................................................................ OBSERV. : PG, ??? , 12 A/MM, 0.28 A INSTRUM.: ESO 1.5M, COUDE; OHP 1.9M, COUDE, 2 A/MM, LALLEMAND EGC LINELIST: ANALYSIS: DIFF(SUN), COG(T-TAU FROM LTE(PEYTREMANN 1970)), T+G(R-I, V-K; IONIZATION FE I/II, TI I/II, CR I/II; ABUNDANCE FROM WEAK AND STRONG LINES; ABSOLUTE MAG.) F-VALUES: DIFF(EPS VIR) REMARKS : ALSO COMPARE OBSERVED AND COMPUTED PROFILES OF NA I D, MG I B LINES COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL, CAYREL 1963: AP.J. 137, 431 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (260) CAYREL, G., CAYREL, R., FOY, R. 1977: ASTRON.ASTROPHYS. 54, 797 ........................................................................ OBSERV. : DATA FROM ( 4) CAYREL, CAYREL 1963: AP.J. 137, 431 INSTRUM.: LINELIST: L, 200 SOLAR F-VALUES (FE I, II; 4510-6800A) ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1970) MODELS), T(VRIK, G-I), G(IONIZATION), T+G(CHECKED WITH NA I D, MG IB LINE PROFILES, ABS.MAG.), F-VALUES: DIFF(SUN) REMARKS : STUDY THE SPLITTING IN THE DAMPING PART OF THE FE COG COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (294) BRANCH, D., BONNELL, J., TOMKIN, J. 1978: ASTROPHYS.J. 225, 902 ........................................................................ OBSERV. : PE, RETICON, 7700-7870A, 8680-8780A, 0.12 A INSTRUM.: MCDONALD 2.7M, ECHELLE LINELIST: LW, 18 ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T+G(LAMBERT, RIES 1977: AP.J. 217, 508) REMARKS : 30 LINES OF ELEMENTS OTHER THAN FE WERE ALSO MEASURED, BUT NOT FULLY ANALYZED COMMENTS: DERIVE FE ABUNDANCE ONLY CLASS : DMA, R ------------------------------------------------------------------------ (290) SNEDEN, C., LAMBERT, D., TOMKIN, J., PETERSON, R.C. 1978: ASTROPHYS.J. 222, 585 ........................................................................ OBSERV. : PG, 4000-4700A, 2 A/MM; 5000-6700A, 5.2 A/MM (LICK); RETICON, 30A SECTIONS CENTERED AT 6300, 6363, 6710, 8000, 8055A, 0.12 A, S/N= 200 (MCDONALD) INSTRUM.: LICK 3.1M, COUDE; MCDONALD, ECHELLE LINELIST: LW, 25: ANALYSIS: LTE(CARBON, GINGERICH 1969; GUSTAFSSON), DIFF(SUN), T(UBVRI, 2.3+3.6 MU; LINE EXCITATION), G(IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (319) HEARNSHAW, J.B., NEWBURGH, C.D. 1979: MONTHLY NOTICES ROY.ASTRON.SOC. 186, 85 ........................................................................ OBSERV. : PG, 4600-5600A, 4 A/MM INSTRUM.: SAO 1.5M, ECHELLE, KRON EGC LINELIST: 72, LLWW: HEARNSHAW 1977: PUBL.ASTRON.SOC.PACIFIC 89, 356 ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN, DISK CENTRE), T(R-I), G(FE I/II IONIZATION, WINGS OF FE I 5270A LINE) REMARKS : USE ONLY WEAK LINES COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (380) KOMAROV, N.S., SHCHERBAK, A.N. 1980: SOVIET ASTRON. 24, 323 ........................................................................ OBSERV. : PG, 5000-5500A, 14 A/MM INSTRUM.: CRIMEAN AP.OBS. 50-INCH LINELIST: ANALYSIS: COG, DIFF(ALF BOO), T(FE I EXCITATION), PE(FE I/II IONZATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 114710 BET COM F9.5V (EMISS H+K) AR 13 09.5 DEC +28 08 MV = 4.26 FE/H = 0 R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 37) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1963: ASTROPHYS.J. 138, 97 ........................................................................ OBSERV. : PG, 4000-6600A, 2.8+4.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 320: ANALYSIS: COG, DIFF(SUN), EMPIRICAL COG FROM FE I, T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 74) SPINRAD, H., LUEBKE, W.R. 1970: ASTROPHYS.J. 160, 1141 ........................................................................ OBSERV. : PG, 5180-5880A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: COG, DIFF(SUN), T(COLOUR 5360-7400A) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (A20) CORNIDE, M., REGO, M. 1984: ASTROPHYS.SPACE SCI. 105, 55 ........................................................................ OBSERV. : PG, 3900-5000A, 7.2 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: LW, 90 FE I LINES ANALYSIS: LTE(ATLAS), T(R-I, OTHER COLOURS), G(ABS.MAG.+RADIUS/COLOUR RELATION), T+G(TI I,II, FE I,II LINES), F-VALUES: FOY(1972)(DIFF(SUN)), BRIDGES+KORNBLITH) REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : DT(G)MA, L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 114762 BD +18 2700 F9V (SUBDWARF) AR 13 09.9 DEC +17 47 MV = 7.30 FE/H = -- R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15? A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (300) PETERSON, R.C., CARNEY, B.W. 1979: ASTROPHYS.J. 231, 762 ........................................................................ OBSERV. : PG, 5170-5700A, 1.75 A/MM, 0.2 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 140: ANALYSIS: DIFF(SUN), LTE(ATLAS), T(R-I, V-K; SCAN 5000...8400 A), G(ASSUMED), F-VALUES(FE I): BRIDGES+KORNBLITH 1974, MAY ET AL.1974 DIFF(SUN) REMARKS : ANALYZE WEAK FE I LINES COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (300) PETERSON, CARNEY 1979: AP.J. 231, 762 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 115043 BD +57 1425 G1VA (EMISS H+K) AR 13 11.6 DEC +56 58 MV = 6.83 FE/H = 0 L ------------------------------------------------------------------------ ( 29) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1960: ASTROPHYS.J. 132, 553 ........................................................................ OBSERV. : PG, 5150-6270A, 13.5 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTGAA, L ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, LLWW: HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ======================================================================== HD 115383 59 VIR G0VS (EMISS H+K) AR 13 14.3 DEC +09 41 MV = 5.22 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 115444 BD +37 2388 K0 AR 13 14.6 DEC +36 39 MV = 8.5 FE/H = ---- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 117176 70 VIR G4V (EMISS H+K) AR 13 26.0 DEC +14 03 MV = 5.00 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 117440 CD -38 8592 G9IB... AR 13 28.1 DEC -39 09 MV = 3.88 FE/H = - (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6700A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 119796 HR 5171 K0... AR 13 43.7 DEC -62 20 MV = 6.51 FE/H = 0 (R) ------------------------------------------------------------------------ (131) WARREN, P.R. 1973: MONTHLY NOTICES ROY.ASTRON.SOC. 161, 427 ........................................................................ OBSERV. : PG, 5590-6860A, 13.4 A/MM INSTRUM.: RADCLIFFE 1.9M, CASSEGRAIN, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN, EPS VIR), T-TAU SCALED FROM EMPIRICAL SOLAR MODEL(GINGERICH, DE JAGER 1968: SOLAR PHYS. 3, 5) T(LINE EXCITATION), G(IONIZATION) REMARKS : COMMENTS: CLASS : DTMGAA, (R) ======================================================================== HD 120136 TAU BOO F6IV AR 13 44.9 DEC +17 42 MV = 4.50 FE/H = 0 R ------------------------------------------------------------------------ ( 51) SPITE, M. 1968: ANN.ASTROPHYS. 31, 269 ........................................................................ OBSERV. : PG, 4340-6700A, 3.2-12 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 200: ANALYSIS: LTE(T-TAU SCALED FROM SUN: MUTSCHLECNER 1963), DIFF(SUN), T+G(COG OF FE, CR, TI; ABS.MAG.; HALFA, HBETA PROFILES) REMARKS : ALSO ANALYZES PROFILES OF NA I D, MG IB LINES COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : SPITE, M. 1968: ANN.ASTROPHYS. 31, 269 INSTRUM.: LINELIST: 21 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ======================================================================== HD 121370 ETA BOO G0IV AR 13 52.3 DEC +18 39 MV = 2.68 FE/H = 0 R ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : GLEBOCKI, STROBEL 1970: ACTA ASTRON. 20, 361 INSTRUM.: LINELIST: 24 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: SUPERSEDED BY (A14) CLASS : DT(G)MAA ------------------------------------------------------------------------ (A14) TOMKIN, J., LAMBERT, D.L., BALACHANDRAN, S. 1985: ASTROPHYS.J. 290, 289 ........................................................................ OBSERV. : DATA FROM (A24) CLEGG ET AL. 1981: AP.J. 250, 262 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : RE-ANALYSIS OF FE I LINES (CHANGE OF MICROTURBUNLENCE) COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 122563 HR 5270 F8IV (WEAK METALS) AR 14 00.1 DEC +09 56 MV = 6.20 FE/H = ---- R ------------------------------------------------------------------------ ( 26) PAGEL, B.E.J. 1963: J.QUANT.SPECTROSC.RADIAT.TRANSFER 3, 139 ........................................................................ OBSERV. : PG, ??? , 10 A/MM INSTRUM.: RADCLIFFE OBS. LINELIST: 150: ANALYSIS: COG, DIFF(SUN), EMPIRICAL COG FROM FE I LINES T(FE I EXCITATION) REMARKS : TESTS DIFFERENTIAL COG METHOD, PRELIMINARY ANALYSIS COMMENTS: CLASS : (DTAA) ------------------------------------------------------------------------ ( 14) WALLERSTEIN, G., GREENSTEIN, J.L., PARKER, R., HELFER, H.L., ALLER, L.H. 1963: ASTROPHYS.J. 137, 280 ........................................................................ OBSERV. : PG, 3940-6500A, 4.5+6 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN), T(LINE EXCITATION, GRI, SCAN 8000..4000A, IONIZATION) REMARKS : PRELIMINARY ANALYSIS COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 2) PAGEL, B.E.J. 1965: ROY.OBS.BULL. 104 ........................................................................ OBSERV. : DATA FROM ( 14) WALLERSTEIN ET AL.1963: AP.J. 137, 280 INSTRUM.: LINELIST: LLWW, 180: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION, GRI), PE(IONIZATION) REMARKS : TAKES INTO ACCOUNT THE DIFFERENCE IN DAMPING CONSTANTS FOR DIFFERENT MULTIPLETS, AND USES DIFFERENT DIFFERENTIAL EXCITATION TEMPERATURES FOR NEUTRAL AND IONIZED LINES COMMENTS: RE-ANALYSIS: FINDS ZN, SR, YT, ZR ABUND. TO BE SOLAR CLASS : DTAA, L ------------------------------------------------------------------------ ( 83) BALL, C., PAGEL, B.E.J. 1967: OBSERVATORY 87, 19 ........................................................................ OBSERV. : PG, 4100-4900A, 6.7 A/MM INSTRUM.: RADCLIFFE 74-INCH, COUDE LINELIST: LW, 5 (CH LINES) ANALYSIS: COG, DIFF(SUN), T(( 2) PAGEL 1965: R.O.BULL. 104) REMARKS : COMMENTS: DERIVE C ABUNDANCE ONLY CLASS : DA ------------------------------------------------------------------------ ( 79) WOLFFRAM, W. 1972: ASTRON.ASTROPHYS. 17, 17 ........................................................................ OBSERV. : DATA FROM ( 14) WALLERSTEIN ET AL.1963: AP.J. 137, 280 (???) WOLFF ET AL.1967: AP.J. 152, 871 (???) FAWELL 1971: THESIS HERSTMONCEUX INSTRUM.: LINELIST: LLWW, 350 ANALYSIS: LTE, T+G(SCAN 3500..10000A; UBVGRI, UBYV; LINE EXCITATION, IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER 1967 MODEL) REMARKS : FINAL MODEL ALSO REPRODUCES HALFA, HBETA WINGS COMMENTS: USES GREY ATMOSPHERE CF.(419) STEENBOCK 1983: A+A 126, 325 CLASS : DTGMAA ------------------------------------------------------------------------ ( 76) SNEDEN, C. 1973: ASTROPHYS.J. 184, 839 ........................................................................ OBSERV. : PG, 3250-4800A, 9 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: LTE(T-TAU FROM ( 79) WOLFFRAM 1972: A+A 17, 17), SPECTRUM SYNTHESIS, T+G(WOLFFRAM 1972) REMARKS : COMMENTS: DERIVES N ABUNDANCE ONLY CLASS : SA ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3300-3700A, 3800-4700A, 9 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM (328) SPITE SPITE 1979: A+A 76, 150 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN) T(R-I), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (328) SPITE, M., SPITE, F. 1979: ASTRON.ASTROPHYS. 76, 150 ........................................................................ OBSERV. : PG, 4320-4980A, 5250-6220A, 12 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LLWW, 240: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN) T(SCAN 3500-11550A, HBETA, HGAMMA), G(IONIZATION FE, TI, CR) REMARKS : TAKE INTO ACCOUNT VARIATION OF COG WITH EACH IONIC SPECIES: SOME IMPORTANCE FOR NA, MG, BA, Y COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (322) SPITE, M., SPITE, F. 1980: ASTRON.ASTROPHYS. 89, 118 ........................................................................ OBSERV. : PG, 3930-3970A, 7.1 A/MM INSTRUM.: ESO 1.5M, COUDE, ECHELLE, LALLEMAND EGC LINELIST: LW, 4 ANALYSIS: LTE(PEYTREMANN 1974, GUSTAFSSON), DIFF(SUN), T+G(SPITE'S 1979: A+A 76, 150), F-VALUES: WIESE 1969 NSRDS-NBS 22 SPECTRUM SYNTHESIS REMARKS : DERIVE AL ABUNDANCE ONLY COMMENTS: FE AND MG ABUNDANCES ARE QUOTED FROM OTHER WORKS CLASS : DMSA ------------------------------------------------------------------------ (404) BESSELL, M.S., NORRIS, J. 1981: ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS, IAU COLLOQ. NO.68, A.G.D.PHILIP, D.S.HAYES EDS., L.DAVIS PRESS, SCHENECTADY, N.Y., P. 94 ........................................................................ OBSERV. : PE, ??? 5 A/MM INSTRUM.: AAT 3.9M, IPCS LINELIST: 110 ANALYSIS: LTE(GUSTAFSSON, ATLAS), T(BVRI, DDO, UVBY, CMT1T2), T+G(BVRI, DDO, UVBY, CMT1T2; LINE STRENGTH, EXCITATION, IONIZATION), F-VALUES: ABSOLUTE (FE I: BLACKWELL 1980) MOLEK.BANDS: SPECTRUM SYNTHESIS, F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, MT.WILSON 100-INCH, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A27) SNEDEN, C., PARTHASARATHY, M. 1983: ASTROPHYS.J. 267, 757 ........................................................................ OBSERV. : PE, 55A SECTIONS BETWEEN 3400-5000A, 0.13A, S/N= 100 (DIG) 90A SECTIONS BETWEEN 5000-6500A, 0.2A, S/N= >200 (RET) INSTRUM.: MCDONALD 2.7M, COUDE, DIGICON, RETICON LINELIST: LLWW, 450: ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: LABORATORY, AS LISTED; ALSO: COG, DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : FE/H = -2.65 WITH LAB.F-VALUES AND -2.40 WITH SOLAR F-VAL. COMMENTS: CLASS : (D)TGMAA, R ------------------------------------------------------------------------ (419) STEENBOCK, W. 1983: ASTRON.ASTROPHYS. 126, 325 ........................................................................ OBSERV. : WALLERSTEIN ET AL.1963: AP.J. 137, 280 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), DIFF(SUN), T+G(WOLFFRAM 1972: A+A, 17, 17) F-VALUES: DIFF(SUN) REMARKS : REANALYSIS, DERIVES BA, FE, MG ABUNDANCES FROM SELECTED ISOLATED LINES COMMENTS: CLASS : DMA, L ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, V-K, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 122956 BD -14 3867 G5 (WEAK METALS) AR 14 02.5 DEC -14 37 MV = 7.3 FE/H = --- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 123139 TET CEN K0IIIB (EMISS H+K+MG(UV)) AR 14 03.7 DEC -36 07 MV = 2.06 FE/H = 0 R? ------------------------------------------------------------------------ ( 16) WARNER, B. 1965: MONTHLY NOTICES ROY.ASTRON.SOC. 129, 263 ........................................................................ OBSERV. : PG, BLUE RANGE, 6.8 A/MM INSTRUM.: RADCLIFFE 74-INCH, COUDE LINELIST: LW: WARNER 1964: COMM.UNIV.LONDON OBS. 65 ANALYSIS: COG, DIFF(SUN), THEOR.COG. FROM WRUBEL 1949: AP.J. 109, 66 T(COG SHIFTS), PE(IONIZATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 123657 HR 5299 M4.5:III AR 14 05.9 DEC +44 05 MV = 5.27 FE/H = 0 (R) ------------------------------------------------------------------------ (A10) SMITH, V.V., LAMBERT, D.L. 1985: ASTROPHYS.J. 294, 326 ........................................................................ OBSERV. : PE, REGIONS BETWEEN 7330-7600 A, 0.2 A (RETICON) 1.6 + 2.2 MICRON (4500 CM**-1), 0.05 CM**-1 (FTS) INSTRUM.: MCDONALD 2.7M, COUDE, RETICON; KPNO 4M, FTS LINELIST: LW, 29 ATOMIC + 60 MOLECULAR LINES ANALYSIS: LTE(JOHNSON), DIFF(ALF TAU), T(V-K), G(ABS.MAG.+EVOL.TRACKS) F-VALUES: CF. LAMBERT ET AL. 1984: AP.J. 284, 223 REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 124570 14 BOO F6IV AR 14 11.7 DEC +13 12 MV = 5.50 FE/H = 0 R ------------------------------------------------------------------------ (317) GEHREN, T. 1979: ASTRON.ASTROPHYS. 75, 73 ........................................................................ OBSERV. : PG, 4400-6820A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 480:, LLWW: GEHREN ET AL.1978: A+A SUPPL. 31, 297 ANALYSIS: LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), T(LINE PROFILES OF HALFA, HGAMMA), G(IONIZATION SI, TI, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (317) GEHREN 1979: A+A 75, 73 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 124897 ALF BOO K1.5III (EMISS H+K+MG(UV)) AR 14 13.4 DEC +19 27 MV = -0.04 FE/H = - R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ ( 52) GRIFFIN, R., GRIFFIN, R. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 253 ........................................................................ OBSERV. : PG, 5000-7025A, 1+1.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 5000, LLWW: CF. MAECKLE AT AL.1975: A+A SUPPL. 19, 303 ANALYSIS: COG, DIFF(SUN, EPS VIR), T(EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : SAME AS IN REF.(41) INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY REF.(41) DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA ------------------------------------------------------------------------ (181) MAECKLE, R., HOLWEGER, H., GRIFFIN, R., GRIFFIN, R. 1975: ASTRON.ASTROPHYS. 38, 239 ........................................................................ OBSERV. : PG, 5000-8825A, 1 A/MM (GRIFFIN 1968: ARCTURUS ATLAS) INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 1200, LLWW: MAECKLE ET AL.1975: A+A SUPPL. 19, 303 ANALYSIS: LTE(EMPIRICAL T-TAU RELATION DERIVED FROM THE WINGS OF MG I B, NA I D, CA II (IR) FOR TAU .GT. 0.001, STARTING BY SCALING THE EMPIR. SOLAR MODEL OF HOLWEGER 1967: Z.ASTROPHYS. 65, 365), DIFF(SUN), T(SCANS 5000..11000A; PHOTOMETRY: BVRIJK, VBGRI, ...), G(FE I/II, TI I/II, CR I/II, CA I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (282) BLACKWELL, D.E., WILLIS, R.B. 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 180, 169 ........................................................................ OBSERV. : DATA FROM GRIFFIN 1968: ARCTURUS ATLAS INSTRUM.: LINELIST: LW, 20 FE I LINES ANALYSIS: LTE(GUSTAFSSON), T(CONTINUUM 5000-20000A), G(PROFILES OF 7 FE I LINES: 5269..8204A), F-VALUES: LABORATORY, DIFF(SUN), C6-VALUES: DIFF(SUN) REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: THIS WORK EMPHASIZES ON THE DETERMINATION OF GRAVITY CLASS : DTGMA, R ------------------------------------------------------------------------ (271) MARTIN, P. 1977: ASTRON.ASTROPHYS. 61, 591 ........................................................................ OBSERV. : DATA FROM GRIFFIN 1968: ARCTURUS ATLAS INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN, EPS VIR), T(RIJK, G-I, CONTINUUM: 4000..14000A), T+G(FE I/II, TI I/II, CR I/II IONIZATION; WINGS OF NA I D, MG I B, CA II 8542A LINES) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (181) MAECKLE ET AL.1975: A+A SUPPL. 19, 303 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ------------------------------------------------------------------------ (294) BRANCH, D., BONNELL, J., TOMKIN, J. 1978: ASTROPHYS.J. 225, 902 ........................................................................ OBSERV. : PE, RETICON, 7700-7870A, 8680-8780A, 0.12 A INSTRUM.: MCDONALD 2.7M, ECHELLE LINELIST: LW, 18 ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T+G(LAMBERT, RIES 1977: AP.J. 217, 508) REMARKS : 30 LINES OF ELEMENTS OTHER THAN FE WERE ALSO MEASURED, BUT NOT FULLY ANALYZED COMMENTS: DERIVE FE ABUNDANCE ONLY CLASS : DMA, R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ------------------------------------------------------------------------ (A18) BELL, R.A., EDVARDSSON, B., GUSTAFSSON, B. 1985: MONTHLY NOTICES ROY.ASTRON.SOC. 212, 497 ........................................................................ OBSERV. : DATA FROM ARCTURUS ATLAS, MGH DATA FROM TOMKIN, LAMBERT 1976: AP.J. 208, 436 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), G(MGH/MG I, PROFILES OF STRONG FE I, CA I, NA I LINES, FE I/II IONIZATION), T(FRISK ET AL.1982: MNRAS 199, 471), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DGM(A), L ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ------------------------------------------------------------------------ (A17) D'ODORICO, S., GRATTON, R.G., PONZ, D. 1985: ASTRON.ASTROPHYS. 142, 232 ........................................................................ OBSERV. : PE, 5700-6750A, 6 A/MM INSTRUM.: ESO 3.6M, CASSEGRAIN, ECHELLE, CCD LINELIST: LLWW, 120: ANALYSIS: LTE(GUSTAFSSON), T+G(DA COSTA 1981: AP.J. 248, 612: T(V-K), G(ABS.MAG.+ASSUMED MASS)), F-VALUES: KOSTYK ET AL. 1981-83, DIFF(SUN) REMARKS : COMMENTS: CLASS : (D)T(G)MAA, R ======================================================================== HD 125924 BD -07 3835 B2IV AR 14 20.1 DEC -08 01 MV = 9.68 FE/H = -- (R?) ------------------------------------------------------------------------ (A23) TOBIN, W., KAUFMANN, J.P. 1984: MONTHLY NOTICES ROY.ASTRON.SOC. 207, 369 ........................................................................ OBSERV. : PG, 3900-4920A, 49 A/MM; IUE, 1200-3000A, 6+0.02 A INSTRUM.: RADCLIFFE 1.9M, CASSEGRAIN; IUE LINELIST: LW: MICROFICHE MN 207/1 ANALYSIS: LTE(ATLAS), T+G(UBV, UVBY; PROFILES OF HGAMMA, HDELTA, HE I 4471, 4026 A LINES), F-VALUES: ?? REMARKS : COMMENTS: CLASS : TGMAA, (R?) ======================================================================== HD 126587 BD -21 3903 G0 (WEAK METALS) AR 14 24.2 DEC -22 01 MV = 9.13 FE/H = ---- R ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 127665 RHO BOO K3III (EMISS H+K) AR 14 29.7 DEC +30 35 MV = 3.58 FE/H = - (R) ------------------------------------------------------------------------ (254) PILACHOWSKI, C.A. 1977: ASTRON.ASTROPHYS. 54, 465 ........................................................................ OBSERV. : PG, ??? , 3.4-10 A/MM INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LW: TO BE PUBLISHED ??? ANALYSIS: LTE(CARBON, GINGERICH 1969), DIFF(EPS VIR), T(CONT.SLOPE 5400/6300A), G(MG II B LINE PROFILES, FE I/II, TI I/II, CR I/II IONIZATION), F-VALUES: VARIOUS SOURCES REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 128167 SIG BOO F2V (WEAK METALS) AR 14 32.5 DEC +29 58 MV = 4.46 FE/H = - R ------------------------------------------------------------------------ (170) DANZIGER, I.J. 1966: ASTROPHYS.J. 143, 591 ........................................................................ OBSERV. : PG, 3899-4520A, 2.9-7.5 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, DAO LINELIST: 600:, LLWW: WRIGHT ET AL.1964: PUBL.DOM.AP.OBS. 12, 173 ANALYSIS: COG, DIFF(ALF CMI), T(HGAMMA PROFILES), F-VALUES: CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 128279 CD -28 10286 G0 (WEAK METALS) AR 14 33.9 DEC -28 53 MV = 7.97 FE/H = ---- R ------------------------------------------------------------------------ (267) SPITE, M., SPITE, F. 1977: ASTRON.ASTROPHYS.SUPPL. 28, 307 ........................................................................ OBSERV. : PG, 4340-6000A, 12 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LLWW, 240: ANALYSIS: LTE(PEYTREMANN 1970+1974), DIFF(HD 122563, SUN) T(HALFA, HBETA, HGAMMA), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: SUPERSEDED BY (280) SPITE'S 1978: A+A 67, 23 ?? CLASS : DTGMA ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM (267) SPITE SPITE 1977, A+A SUPPL. 28, 307 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(R-I), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DTGMA ------------------------------------------------------------------------ (322) SPITE, M., SPITE, F. 1980: ASTRON.ASTROPHYS. 89, 118 ........................................................................ OBSERV. : PG, 3930-3970A, 7.1 A/MM INSTRUM.: ESO 1.5M, COUDE, ECHELLE, LALLEMAND EGC LINELIST: LW, 4 ANALYSIS: LTE(PEYTREMANN 1974, GUSTAFSSON), DIFF(SUN), T+G(SPITE'S 1978: A+A 67, 23), F-VALUES: WIESE 1969 NSRDS-NBS 22 SPECTRUM SYNTHESIS REMARKS : DERIVE AL ABUNDANCE ONLY COMMENTS: FE AND MG ABUNDANCES ARE QUOTED FROM OTHER WORKS CLASS : DMSA ======================================================================== HD 128620 ALF1 CEN G2V AR 14 36.2 DEC -60 38 MV = -0.01 FE/H = 0 R ------------------------------------------------------------------------ ( 80) FRENCH, V.A., POWELL, A.L.T. 1971: ROY.OBSERV.BULL.GREENWICH 173 ........................................................................ OBSERV. : PG, 4200-6850A, 6.7 A/MM; 5580-6750A, 2.5 A/MM INSTRUM.: MT.STROMLO 74-INCH, COUDE LINELIST: LLWW, 921 ANALYSIS: COG(VAN DER HELD TYPE COG SHAPE), DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (338) ENGLAND, M.N. 1980: MONTHLY NOTICES ROY.ASTRON.SOC. 191, 23 ........................................................................ OBSERV. : PG, 4800-6650A, 1.8 A/MM INSTRUM.: MT.JOHN UNIV.OBS. 0.6M, CASSEGRAIN, ECHELLE LINELIST: 289 ANALYSIS: LTE(SCALED FROM SEMI-EMPIRICAL SOLAR MODEL VAL (1976), EXTENDED BY SOLAR MODEL PEYTREMANN 1974), DIFF(SUN), T+G(FE I/II IONIZATION; PARALLAX + BINARY MASS; PROFILES OF HALFA, FE I 5269A) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 128621 ALF2 CEN K1V (EMISS H+K) AR 14 36.2 DEC -60 38 MV = 1.33 FE/H = 0 R ------------------------------------------------------------------------ ( 80) FRENCH, V.A., POWELL, A.L.T. 1971: ROY.OBSERV.BULL.GREENWICH 173 ........................................................................ OBSERV. : PG, 4200-6850A, 6.7 A/MM; 5290-6770, 2.5 A/MM INSTRUM.: MT.STROMLO 74-INCH, COUDE LINELIST: LLWW, 1029 ANALYSIS: COG(VAN DER HELD TYPE COG SHAPE), DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (338) ENGLAND, M.N. 1980: MONTHLY NOTICES ROY.ASTRON.SOC. 191, 23 ........................................................................ OBSERV. : PG, 4800-6650A, 1.8 A/MM INSTRUM.: MT.JOHN UNIV.OBS. 0.6M, CASSEGRAIN, ECHELLE LINELIST: 289 ANALYSIS: LTE(SCALED FROM SEMI-EMPIRICAL SOLAR MODEL VAL (1976), EXTENDED BY SOLAR MODEL PEYTREMANN 1974), DIFF(SUN), T+G(FE I/II IONIZATION; PARALLAX + BINARY MASS; PROFILES OF HALFA, FE I 5269A) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 128959 CD -26 10427 F7V (WEAK METALS) AR 14 37.8 DEC -26 31 MV = 9.25 FE/H = -- (R) ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 130095 CD -26 10505 A0V (HORIZONTAL BRANCH) AR 14 43.9 DEC -27 02 MV = 8.13 FE/H = -- R ------------------------------------------------------------------------ (405) KODAIRA, K., PHILIP, A.G.D. 1981: ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS, IAU COLLOQ. NO.68, A.G.D.PHILIP, D.S.HAYES EDS., L.DAVIS PRESS, SCHENECTADY, N.Y., P. 153 ........................................................................ OBSERV. : ??? 12.5 A/MM ?? INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: ANALYSIS: LTE(ATLAS), T+G(PHOTOMETRY, HDELTA PROFILE) REMARKS : GIVE FE/H ONLY COMMENTS: SUPERSEDED BY (A22) CLASS : TGMA ------------------------------------------------------------------------ (A22) KODAIRA, K., PHILIP, A.G.D. 1984: ASTROPHYS.J. 278, 208 ........................................................................ OBSERV. : PG, 3850-4300A, 12.5 A/MM INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), DIFF(HD 161817), T+G(B-V, C1, M1, HDELTA WING), F-VALUES: KURUCZ+PEYTREMANN 1975 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 130227 HR 5515 K1III AR 14 45.4 DEC -56 28 MV = 6.23 FE/H = - (L) ------------------------------------------------------------------------ (239) WEGNER, G. 1976: MONTHLY NOTICES ROY.ASTRON.SOC. 177, 3 ........................................................................ OBSERV. : PG, 4554-5002A, 6.8 A/MM INSTRUM.: RADCLIFFE 1.9M, COUDE LINELIST: 125 ANALYSIS: COG, DIFF(ALF BOO), T(UBVRI, R-I), PE(TI I/II IONIZATION) F-VALUES FROM ARCTURUS ATLAS(GRIFFIN 1968) REMARKS : COMMENTS: CLASS : DTA, (L) ======================================================================== HD 130694 58 HYA K4III AR 14 47.3 DEC -27 45 MV = 4.42 FE/H = - (L) ------------------------------------------------------------------------ (239) WEGNER, G. 1976: MONTHLY NOTICES ROY.ASTRON.SOC. 177, 3 ........................................................................ OBSERV. : PG, 4554-5002A, 6.8 A/MM INSTRUM.: RADCLIFFE 1.9M, COUDE LINELIST: 125 ANALYSIS: COG, DIFF(ALF BOO), T(UBVRI, R-I), PE(TI I/II IONIZATION) F-VALUES FROM ARCTURUS ATLAS(GRIFFIN 1968) REMARKS : COMMENTS: CLASS : DTA, (L) ======================================================================== HD 130952 11 LIB G8III (EMISS H+K) AR 14 48.4 DEC -02 06 MV = 4.94 FE/H = 0 L ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, L ======================================================================== HD 131156 XI BOO G8V (EMISS H+K) AR 14 49.1 DEC +19 18 MV = 4.55 FE/H = 0 L ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 4.5+6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (A20) CORNIDE, M., REGO, M. 1984: ASTROPHYS.SPACE SCI. 105, 55 ........................................................................ OBSERV. : PG, 3900-5000A, 7.2 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: LW, 90 FE I LINES ANALYSIS: LTE(ATLAS), T(R-I, OTHER COLOURS), G(ABS.MAG.+RADIUS/COLOUR RELATION), T+G(TI I,II, FE I,II LINES), F-VALUES: FOY(1972)(DIFF(SUN)), BRIDGES+KORNBLITH) REMARKS : DERIVE FE/H ONLY COMMENTS: CLASS : DT(G)MA, L ======================================================================== HD 131977 HR 5568 K5V (EMISS H+K) AR 14 54.5 DEC -21 11 MV = 5.74 FE/H = 0 (R) ------------------------------------------------------------------------ (246) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 85 ........................................................................ OBSERV. : PG, EGC, 4650-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE LINELIST: LLWW, 200: ANALYSIS: DIFF(SUN), LTE(PEYTREMANN 1974), T(R-I, I-K), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUND. ONLY COMMENTS: CF. HEARNSHAW 1976: A.A. 51, 71 CLASS : DTGMA, (R) ======================================================================== HD 132142 BD +54 1716 K1V AR 14 53.8 DEC +53 53 MV = 7.73 FE/H = -- (R) ------------------------------------------------------------------------ (300) PETERSON, R.C., CARNEY, B.W. 1979: ASTROPHYS.J. 231, 762 ........................................................................ OBSERV. : PG, 5170-5700A, 1.75 A/MM, 0.2 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 140: ANALYSIS: DIFF(SUN), LTE(ATLAS), T(R-I, V-K; SCAN 5000...8400 A), G(ASSUMED), F-VALUES(FE I): BRIDGES+KORNBLITH 1974, MAY ET AL.1974 DIFF(SUN) REMARKS : ANALYZE WEAK FE I LINES COMMENTS: CLASS : DTGMA, (R) ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM PETERSON, CARNEY 1979: AP.J. 231, 762 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 132345 18 LIB K3IIICN... (CN) AR 14 56.2 DEC -10 57 MV = 5.87 FE/H = 0 (L) ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, (L) ======================================================================== HD 132475 BD -21 4009 F7V-VI (WEAK METALS, SUBDWARF) AR 14 57.0 DEC -21 48 MV = 8.57 FE/H = --- R ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : PG, 4500-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, EGC LINELIST: LLWW, 50: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), LTE(ATLAS), DIFF(SUN), T(R-I), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : DATA FROM (245) HEARNSHAW 1976: A+A 51, 71 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION) REMARKS : REANALYSIS COMMENTS: CLASS : DGMA, R ======================================================================== HD 134169 BD +04 2969 G1VM (WEAK METALS) AR 15 05.8 DEC +04 07 MV = 7.70 FE/H = --- R? ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3300-3700A, 18A/MM, 3800-4700A, 9+18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, L ------------------------------------------------------------------------ (302) SNEDEN, C., LAMBERT, D.L., WHITAKER, R.W. 1979: ASTROPHYS.J. 234, 964 ........................................................................ OBSERV. : PG, ???? , 9 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: DAOR ANALYSIS: LTE(PEYTREMANN 1974?), T(B-Y, FE I EXCITATION), G(FE, CR, TI, V IONIZATION), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: THIS PAPER DEALS WITH THE DERIVATION OF O ABUNDANCES ONLY. IT BRIEFLY RELATES THE FULL ANALYSIS THE RESULTS OF WHICH ARE QUOTED: TEFF, G, MICRO, FE/H CLASS : DTGMA, R? ======================================================================== HD 134439 BD -15 4042 K0V (SUBDWARF, WEAK METALS) AR 15 07.5 DEC -16 08 MV = 9.07 FE/H = --- (R) ------------------------------------------------------------------------ (333) CARNEY, B.W., PETERSON, R.C. 1981: ASTROPHYS.J. 245, 238 ........................................................................ OBSERV. : PG, 3900-5300A, 5.1 A/MM, 0.28 A INSTRUM.: CTIO 4M, CASSEGRAIN, ECHELLE, IT LINELIST: LLWW, 90: ANALYSIS: LTE(ATLAS), T(SCAN PASCHEN CONT.), G(ADOPTED), F-VALUES: FURNACE(BLACKWELL ET AL.1980) REMARKS : COMMENTS: CLASS : TMAA, (R) ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (333) CARNEY, PETERSON 1981: AP.J. 245, 238 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 134440 BD -15 4041 K3V-VI (SUBDWARF, WEAK METALS) AR 15 07.5 DEC -16 13 MV = 9.44 FE/H = --- (R) ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : PG, PORTIONS IN THE RANGE 4600-6600A, 0.28 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: LLWW, LESS THAN 150: ANALYSIS: LTE(ATLAS), T(R-I, V-K), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVES FE/H ONLY COMMENTS: CLASS : DTGMA, (R) ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 5250-6680A, 5.5 A/MM, 0.29 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: 150:, LLWW: PETERSON 1979: ASTROPHYS.J. 235, 491 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 134678 BD +77 571 F7VM (WEAK METALS) AR 15 05.2 DEC +77 34 MV = 7.66 FE/H = - (R?) ------------------------------------------------------------------------ (302) SNEDEN, C., LAMBERT, D.L., WHITAKER, R.W. 1979: ASTROPHYS.J. 234, 964 ........................................................................ OBSERV. : PG, ???? , 9 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: DAOR ANALYSIS: LTE(PEYTREMANN 1974?), T(B-Y, FE I EXCITATION), G(FE, CR, TI, V IONIZATION), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: THIS PAPER DEALS WITH THE DERIVATION OF O ABUNDANCES ONLY. IT BRIEFLY RELATES THE FULL ANALYSIS THE RESULTS OF WHICH ARE QUOTED: TEFF, G, MICRO, FE/H CLASS : DTGMA, (R?) ======================================================================== HD 135148 BD +12 2804 K0 (WEAK METALS) AR 15 10.9 DEC +12 39 MV = 9.4 FE/H = --- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 5200-6800A, 2.3 A/MM, 0.1A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 135722 DEL BOO G8III (EMISS H+K, CN) AR 15 13.5 DEC +33 30 MV = 3.47 FE/H = - R ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 43) HELFER 1968: AP.J.SUPPL. 16, 1 INSTRUM.: LINELIST: ANALYSIS: DIFF(MEAN OF GAM TAU, DEL TAU, EPS TAU, EPS VIR), LTE(ATLAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 136064 HR 5691 F9IV AR 15 14.0 DEC +67 32 MV = 5.10 FE/H = 0 (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 136202 5 SER F8III-IV AR 15 16.8 DEC +01 57 MV = 5.10 FE/H = 0 R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 90) ZIELKE, G. 1970: ASTRON.ASTROPHYS. 6, 206 ........................................................................ OBSERV. : PG, 3900-4800A, 10 A/MM; 4800-6700A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LESS THAN 600:, LLWW: ZIELKE 1970: A+A SUPPL. 2, 205 ANALYSIS: LTE(T-TAU SCALED FROM SUN: HOLWEGER 1967: Z.AP. 65, 365), T(PROFILES OF HALFA, HBETA, HGAMMA, HDELTA; BVGRI; LINE EXCITATION), G(IONIZATION SI, SC, TI, V, CR, FE, SR), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : POWELL 1971: ROY.OBS.BULL. 167 INSTRUM.: LINELIST: 9 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(BVRIJK), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : T(M)A, L ======================================================================== HD 136352 NU2 LUP G4V AR 15 18.4 DEC -48 08 MV = 5.65 FE/H = - R ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I, SCAN), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, R ======================================================================== HD 136512 OMI CRB K0III AR 15 18.0 DEC +29 48 MV = 5.51 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5280-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 137759 IOT DRA K2III (EMISS H+K) AR 15 23.8 DEC +59 08 MV = 3.29 FE/H = 0 (R) ------------------------------------------------------------------------ (140) WILLIAMS, P.M. 1974: MONTHLY NOTICES ROY.ASTRON.SOC. 167, 359 ........................................................................ OBSERV. : PG, 4720-5240A, 2.2 A/MM INSTRUM.: RGO I.N.T., COUDE LINELIST: LLWW, 140: ANALYSIS: LTE(SCALED SOLAR MODELS(HSRA)), DIFF(EPS VIR), T+G(B-V, I-K; FE I EXCITATION; FE, TI IONIZATION; ABS.MAG.+THEOR. MASS-LUMINOS.REL.) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ------------------------------------------------------------------------ (217) PETERSON, R.C. 1976: ASTROPHYS.J.SUPPL. 30, 61 ........................................................................ OBSERV. : PG, 5190-5890A, 1.7 A/MM INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 210: ANALYSIS: NO ANALYSIS WAS PERFORMED REMARKS : COMMENTS: CLASS : ======================================================================== HD 138716 37 LIB K1IV (EMISS H+K) AR 15 31.4 DEC -09 54 MV = 4.61 FE/H = 0 (L) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (L) ======================================================================== HD 138764 HR 5780 B6IV AR 15 31.7 DEC -09 01 MV = 5.17 FE/H = 0 (R) ------------------------------------------------------------------------ (A25) ADELMAN, S.J. 1984: MONTHLY NOTICES ROY.ASTRON.SOC. 206, 637 ........................................................................ OBSERV. : PG, ??? , 4.3 A/MM INSTRUM.: MT.WILSON LINELIST: 50:, LW: MICROFICHE MN 206/1 ANALYSIS: LTE(ATLAS), DIFF(SUN), T+G(SCAN 3300-7100A, HGAMMA PROFILE), F-VALUES: BLACKWELL, KORNBLITH+BRIDGES, AND OTHERS REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 138905 GAM LIB G8III (EMISS H+K) AR 15 32.7 DEC -14 37 MV = 3.91 FE/H = - (L) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (L) ======================================================================== HD 139669 TET UMI K5III AR 15 32.9 DEC +77 31 MV = 4.96 FE/H = 0 (L) ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, (L) ======================================================================== HD 140283 BD -10 4149 F3VI (WEAK METALS, SUBDWARF) AR 15 40.4 DEC -10 46 MV = 7.20 FE/H = ---- R ------------------------------------------------------------------------ ( 11) CHAMBERLAIN, J.W., ALLER, L.H. 1951: ASTROPHYS.J. 114, 52 ........................................................................ OBSERV. : PG, 4064-4732A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 65: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66), LTE MODELS, F-VALUES: KING 1938+42, T+G(FE I/II IONIZATION, PROFILES OF HBETA, HGAMMA, HDELTA, AND CA I K LINES) REMARKS : DERIVE FE AND CA ABUNDANCES COMMENTS: CLASS : TG(M)A ------------------------------------------------------------------------ ( 7) BASCHEK, B. 1959: Z.ASTROPHYS. 48, 95 ........................................................................ OBSERV. : PG, 3430-4870A, 10 A/MM; 4830-8750A, 20 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 340: ANALYSIS: COG(WEIGHTING FUNCTIONS FROM LTE MODEL(T-TAU DERIVED A LA HUNGER, TRAVING 1956: Z.ASTROPHYS. 39, 248; COG SHAPE FROM: HUNGER 1956: Z.ASTROPHYS. 39, 36), T(UVBGRI, PROFILES OF HALFA..HDELTA), G( CA I/II IONIZ.), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ ( 38) ALLER, L.H., GREENSTEIN, J.L. 1960: ASTROPHYS.J.SUPPL. 5, 139 ........................................................................ OBSERV. : PG, 3650-4900A, 10 A/MM, 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE, MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 65: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66), T(SOLAR EXC.TEMP. ASSUMED), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : D(T)AA, L ------------------------------------------------------------------------ ( 58) COHEN, J.G., STROM, S.E. 1968: ASTROPHYS.J. 151, 623 ........................................................................ OBSERV. : DATA FROM ALLER, GREENSTEIN 1960: AP.J.SUPPL. 5, 139 INSTRUM.: LINELIST: ANALYSIS: LTE(STROM ET AL.1966: AP.J. 146, 880), T(CONT, HGAMMA, CF. STROM ET AL.1966: AP.J. 147, 1038), G(EVOLUT. TRACKS), T+G CHECKED BY FE EXCITATION+IONIZATION F-VALUES: CHECKED WITH SOLAR LINES REMARKS : COMMENTS: CLASS : (D)TGAA, L ------------------------------------------------------------------------ (244) GRABOWSKI, B. 1976: ACTA ASTRON. 26, 147 ........................................................................ OBSERV. : PG, 3600-4500A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG(WEIGHTING FUNCTIONS FROM LTE(CAYREL, JUGAKU) MODELS; COG SHAPE FROM SUN(COWLEY'S 1964: AP.J. 140, 713), UNSOELD 1968: STERNATMOSPHAEREN), DIFF(SUN), T(FE I EXCITATION; TI I/II IONIZATION, NE FROM BALMER LINES VIA INGLIS-TELLER FORMULA; HGAMMA PROFILE), F-VALUES: VARIOUS WORKS(1964-1975) AS LISTED REMARKS : COMMENTS: CLASS : DTMAA, L ------------------------------------------------------------------------ (283) PETERSON, R.C. 1976: ASTROPHYS.J. 206, 800 ........................................................................ OBSERV. : PG, 3940-4760A, 1.5 A/MM INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), T(FE I EXCITATION), G(TI I/II IONIZATION), F-VALUES: FE I: BRIDGES, KORNBLITH 1974: AP.J. 192, 793 REMARKS : CHECK OF THE LABORATORY F-VALUES FOR FE I YIELDED A SIGNIFICANT DISAGREEMENT. COMMENTS: CLASS : TGMAA, R ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM PETERSON 1976: AP.J. 206, 800 INSTRUM.: LINELIST: USE LINES LONGWARD OF 4300 A ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(PETERSON), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (300) PETERSON, R.C., CARNEY, B.W. 1979: ASTROPHYS.J. 231, 762 ........................................................................ OBSERV. : PG, 5170-5700A, 1.75 A/MM, 0.2 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 100: ANALYSIS: DIFF(SUN), LTE(ATLAS), T(R-I, V-K; SCAN 5000...8400 A), G(ASSUMED), F-VALUES(FE I): BRIDGES+KORNBLITH 1974, MAY ET AL.1974 DIFF(SUN) REMARKS : ANALYZE WEAK FE I LINES COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (322) SPITE, M., SPITE, F. 1980: ASTRON.ASTROPHYS. 89, 118 ........................................................................ OBSERV. : PG, 3930-3970A, 7.1 A/MM INSTRUM.: ESO 1.5M, COUDE, ECHELLE, LALLEMAND EGC LINELIST: LW, 4 ANALYSIS: LTE(PEYTREMANN 1974, GUSTAFSSON), DIFF(SUN), T+G(SPITE'S 1978: A+A 67, 23), F-VALUES: WIESE 1969 NSRDS-NBS 22 SPECTRUM SYNTHESIS REMARKS : DERIVE AL ABUNDANCE ONLY COMMENTS: FE AND MG ABUNDANCES ARE QUOTED FROM OTHER WORKS CLASS : DMSA ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 5170-5700A, 1.91 A/MM, 0.22 A INSTRUM.: SAO 1.5M, ECHELLE, EGC LINELIST: 18:, LLWW: PETERSON, CARNEY 1979: ASTROPHYS.J. 231, 762 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES MG, AL ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ------------------------------------------------------------------------ (A13) MAGAIN, P. 1985: ASTRON.ASTROPHYS. 132, 208 ........................................................................ OBSERV. : PG, 4000-4900A, 12.4 A/MM, 0.25 A, 10 COADDED SPECTRA, S/N= 100..200 INSTRUM.: OHP 1.5M, COUDE LINELIST: LW, 33 ANALYSIS: LTE(GUSTAFSON, EMPIRICAL T(TAU) RELATION FROM SCAN 4000..8000A, HGAMMA, HDELTA PROFILES)), T(R-I, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: LABORATORY(BLACKWELL 1982) REMARKS : USES ONLY LINES WITH EQUIV.WIDTHS 10..100 MA COMMENTS: EMPIRICAL TEMPERATURE(TAU) RELATION STEEPER THAN FROM GUSTAFSSON MODEL IN LAYERS DEEPER THAN TAU= 1 SUPERSEDED BY (A12) CLASS : TGMA ------------------------------------------------------------------------ (A12) MAGAIN, P. 1985: ASTRON.ASTROPHYS. 146, 95 ........................................................................ OBSERV. : DATA FROM (A13) MAGAIN 1985: A+A 132, 208, AND PG, 3700-4900A, 12.4 A/MM, 16 SPECTRA COADDED INSTRUM.: ESO 1.5M, COUDE LINELIST: LLWW, 160: ANALYSIS: LTE(EMPIRICAL T(TAU) FROM SCAN 4000-1000A), T(SCAN 4000-9000A, UV SHORTER THAN 3080A, V-K), G(FE I/II, TI I/II IONIZATION; STRONG LINES OF FE I, CA I; PROFILES OF CA II K, BALMER LINES; BJ), F-VALUES: LABORATORY(BLACKWELL 1982) REMARKS : EXTENSION OF (A13) COMMENTS: CLASS : TGMAA, R ======================================================================== HD 140573 ALF SER K2IIIB AR 15 41.8 DEC +06 35 MV = 2.65 FE/H = 0 R? ------------------------------------------------------------------------ ( 60) GRIFFIN, R. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 143, 223 ........................................................................ OBSERV. : PG, 5640-6320A, 1.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 2000 ANALYSIS: COG(EMPIRICAL COG), DIFF(ALF BOO), T(FE I, TI I EXCITATION) REMARKS : PRELIMINARY STUDY COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.4+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 141004 LAM SER G0V AR 15 44.0 DEC +07 31 MV = 4.43 FE/H = 0 R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (317) GEHREN, T. 1979: ASTRON.ASTROPHYS. 75, 73 ........................................................................ OBSERV. : PG, 4400-6820A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 480:, LLWW: GEHREN ET AL.1978: A+A SUPPL. 31, 297 ANALYSIS: LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), T(LINE PROFILES OF HALFA, HBETA, HGAMMA), G(IONIZATION SI, TI, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (317) GEHREN 1979: A+A 75, 73 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 141714 DEL CRB G3.5III (EMISS H+K) AR 15 47.5 DEC +26 13 MV = 4.63 FE/H = 0 (L) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (L) ======================================================================== HD 142198 TET LIB G8.8IIIB (EMISS H+K) AR 15 51.0 DEC -16 35 MV = 4.15 FE/H = 0 (L) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (L) ======================================================================== HD 142267 39 SER G0V AR 15 50.9 DEC +13 21 MV = 6.10 FE/H = - (L) ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 142373 KHI HER F8VE AR 15 50.9 DEC +42 35 MV = 4.62 FE/H = - R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM, 5800-6800A, 6.8 A/MM INSTRUM.: RGO 30-INCH, COUDE, MT.WILSON 100-INCH, COUDE LINELIST: 300:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (317) GEHREN, T. 1979: ASTRON.ASTROPHYS. 75, 73 ........................................................................ OBSERV. : PG, 4400-6820A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 480:, LLWW: GEHREN ET AL.1978: A+A SUPPL. 31, 297 ANALYSIS: LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), T(LINE PROFILES OF HALFA, HBETA, HGAMMA), G(IONIZATION SI, TI, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (317) GEHREN 1979: A+A 75, 73 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 142860 GAM SER F6IV AR 15 54.1 DEC +15 49 MV = 3.85 FE/H = 0 R ------------------------------------------------------------------------ ( 8) KEGEL, W.H. 1962: Z.ASTROPHYS. 55, 221 ........................................................................ OBSERV. : PG, 4200-6773A, 4.6+6.9 A/MM; 6890-8690A, 20 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 1800: FEATURES 3863-8689A, 280: LINES FOR ABUND.ANAL. ANALYSIS: LTE(T-TAU DERIVED A LA HUNGER, TRAVING 1956: Z.AP. 39, 248) T+G(EXCITATION; CA I/II, FE I/II, TI I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED, COMPARES OBSERVED UVBGRI COLOURS, PROFILES OF HALFA..HGAMMA WITH MODEL VALUES REMARKS : COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ ( 55) SPITE, M. 1967: ANN.ASTROPHYS. 31, 685 ........................................................................ OBSERV. : DATA FROM ( 8) KEGEL 1962: Z.AP. 55, 221 INSTRUM.: LINELIST: ANALYSIS: LTE(T-TAU SCALED FROM SUN(MUTSCHLECNER 1963: THESIS)), DIFF(SUN), T(FE, TI, CR EXCITATION, IONIZATION; ABSOL.MAG. + EVOL.TRACKS), COMPARES OBSERVED PROFILES OF HALFA..HGAMMA, WIDTHS OF CA II TRIPLET LINES WITH MODEL VALUES REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 144921 SX HER K2 (WEAK METALS) AR 16 05.3 DEC +25 02 MV = -.-- FE/H = --- (R) ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 6.8 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE, IT LINELIST: 50 ANALYSIS: DIFF(SUN, EPS VIR), COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 143761 RHO CRB G0VA AR 15 59.1 DEC +33 27 MV = 5.40 FE/H = 0 R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA, L ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 145544 DEL TRA G2IB-II (EMISS H+K) AR 16 10.9 DEC -63 34 MV = 3.80 FE/H = 0 (R) ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5700-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON,; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 145675 14 HER K0V (EMISS H+K) AR 16 08.8 DEC +43 57 MV = 6.67 FE/H = 0 R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 4.5+6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), THEOR. COG FROM LTE MODELS(PEYTREMANN 1970), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (246) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 85 ........................................................................ OBSERV. : PG, EGC, 4650-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE LINELIST: LLWW, 200: ANALYSIS: DIFF(SUN), LTE(PEYTREMANN 1974) T(R-I, SCAN 5000-10800A(OINAS 1974)) G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUND. ONLY COMMENTS: CF. HEARNSHAW 1976: A.A. 51, 71 CLASS : DTGMA, R ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ------------------------------------------------------------------------ (289) PETERSON, R.C. 1978: ASTROPHYS.J. 224, 595 ........................................................................ OBSERV. : PG, 4830-5520A, 1.8 A/MM, 0.07 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LW, 90: ANALYSIS: LTE(ATLAS), DIFF(SUN(HSRA), 70 OPH A), T(FE I, CO I, NI I EXCITATION), G(CR I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED, FE I/II: DIFF(SUN), REMARKS : TEFF CHECKED WITH R-I COLOUR COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 146051 DEL OPH M0.5III (EMISS H+K) AR 16 11.7 DEC -03 34 MV = 2.74 FE/H = 0 (L) ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : PG, ?????, 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH LINELIST: 250 ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, (L) ======================================================================== HD 146233 18 SCO G2VA AR 16 12.9 DEC -08 14 MV = 5.50 FE/H = 0 (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 147394 TAU HER B5IV AR 16 18.3 DEC +46 26 MV = 3.89 FE/H = + (R) ------------------------------------------------------------------------ (278) ADELMAN, S.J. 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 667 ........................................................................ OBSERV. : PG, 3820-6680A, 4.3+6.7+8.9+10.4 A/MM INSTRUM.: KPNO, MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 70: ANALYSIS: LTE(ATLAS), DIFF(SUN(HSRA), 70 OPH A), T+G(SCAN 3300..7100A, HGAMMA PROFILE), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : TGMAA, (R) ======================================================================== HD 148387 ETA DRA G8III (EMISS H+K) AR 16 23.3 DEC +61 38 MV = 2.74 FE/H = 0 R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 148783 30 HER M6III (EMISS H+K) AR 16 27.0 DEC +41 59 MV = 5.0 FE/H = 0 (R) ------------------------------------------------------------------------ (A10) SMITH, V.V., LAMBERT, D.L. 1985: ASTROPHYS.J. 294, 326 ........................................................................ OBSERV. : PE, REGIONS BETWEEN 7330-7600 A, 0.2 A (RETICON) 1.6 + 2.2 MICRON (4500 CM**-1), 0.05 CM**-1 (FTS) INSTRUM.: MCDONALD 2.7M, COUDE, RETICON; KPNO 4M, FTS LINELIST: LW, 29 ATOMIC + 60 MOLECULAR LINES ANALYSIS: LTE(JOHNSON), DIFF(ALF TAU), T(V-K), G(ABS.MAG.+EVOL.TRACKS) F-VALUES: CF. LAMBERT ET AL. 1984: AP.J. 284, 223 REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 148816 BD +04 3195 F8V (SUBDWARF) AR 16 28.0 DEC +04 18 MV = 7.27 FE/H = -- R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : PG, PORTIONS IN THE RANGE 4600-6600A, 0.28 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: LLWW, LESS THAN 150: ANALYSIS: LTE(ATLAS), T(R-I, V-K), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVES FE/H ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 5250-6680A, 5.5 A/MM, 0.29 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: 150:, LLWW: PETERSON 1979: ASTROPHYS.J. 235, 491 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 148856 BET HER G7IIIA (EMISS H+K+MG(UV)) AR 16 28.1 DEC +21 36 MV = 2.77 FE/H = 0 L ------------------------------------------------------------------------ ( 47) GRIFFIN, R. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 413, 381 ........................................................................ OBSERV. : PG, 5190-6260A, 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 600: ANALYSIS: COG(EMPIR. FROM ALF BOO), DIFF(ALF BOO), T(FE I , TI I EXCITATION; RIJKL), PE( FI, FE IONIZATION), F-VALUES: DIFF(ALF BOO) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (380) KOMAROV, N.S., SHCHERBAK, A.N. 1980: SOVIET ASTRON. 24, 323 ........................................................................ OBSERV. : PG, 5000-5500A, 14 A/MM INSTRUM.: CRIMEAN AP.OBS. 50-INCH LINELIST: ANALYSIS: COG, DIFF(ALF BOO), T(FE I EXCITATION), PE(FE I/II IONZATION) REMARKS : COMMENTS: CLASS : DTAA, L ======================================================================== HD 149382 BD -03 3967 B5 AR 16 31.8 DEC -03 55 MV = 8.95 FE/H = --- R ------------------------------------------------------------------------ (A03) BASCHEK, B., NORRIS, J. 1975: ASTROPHYS.J. 199, 694 ........................................................................ OBSERV. : PG, 6300-4800A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 17 ANALYSIS: LTE(ATLAS UNBLANK.), T+G(UBV, BJ, HGAMMA WINGS, LAST VISIBLE BALMER LINE; EXTRAPOLATE RESULTS FROM NLTE(MIHALAS 1972) MODELS) COMPARE OBS. AND CALC. HDELTA, HGAMMA PROFILES, SCAN 5000..3300A F-VALUES: DIFF(TAU SCO) REMARKS : COMMENTS: CLASS : DTGM(N)A, L ------------------------------------------------------------------------ (A05) BASCHEK, B., KUDRITZKI, R.-P., SCHOLZ, M., SIMON, K.P. 1982: ASTRON.ASTROPHYS. 108, 387 ........................................................................ OBSERV. : 1160-3230A, 0.2A PLUS DATA FROM BASCHEK, NORRIS 1975: AP.J. 199, 694 INSTRUM.: IUE LINELIST: LLWW, 260: (1500 FEATURES FOUND) ANALYSIS: NLTE(KUDRITZKI, PURE H+HE), LTE(HEAVIER ELEMENTS), T+G(HGAMMA, HDELTA, HE I 4471, 4026, HE II 4686A STRENGTHS) WIDTHS OF HALFA..H8), F-VALUES: VARIOUS SOURCES AS LISTED, COMPARE OBSERVED AND CALC.PROFILES OF HGAMMA, HDELTA, HE I 4471, 4026, HE II 4686 A REMARKS : COMMENTS: CLASS : TGMNAA, R ======================================================================== HD 149438 TAU SCO B0V AR 16 32.8 DEC -28 07 MV = 2.82 FE/H = ? L ------------------------------------------------------------------------ (119) SCHOLZ, M. 1967: Z.ASTROPHYS. 65, 1 ........................................................................ OBSERV. : PG, 3324-3994A, 2 A/MM; 3990-4294A, 1 A/MM; 4921-6721A, 6.5 A/MM; 6560-8598A, 41 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 800:, LLWW: SCHOLZ 1965: ASTRON.ABH.HAMBURG.STERNW. 7, 321 ANALYSIS: LTE(UNBLANKETED), T+G(C II/III, N II/III, SI III/IV IONIZATION; WIDTHS OF HALFA..H8), F-VALUES: VARIOUS SOURCES AS LISTED, COMPARES OBSERVED AND CALC.PROFILES OF HGAMMA, HDELTA, HE I 4438, 4121, O II 4649, 4317, 4076, N II 4447, MG II 4481 A REMARKS : COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ (105) HARDORP, J., SCHOLZ, M. 1970: ASTROPHYS.J.SUPPL. 19, 193 ........................................................................ OBSERV. : PG, 3220-6700A, 1..6.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 420: ANALYSIS: LTE(MIHALAS 1965), T+G(BALMER JUMP; IONIZATION C, N, SI; HGAMMA, HDELTA PROF.) CHECKED WITH SCAN 3300-6500A, F-VALUES: VARIOUS SOURCES AS QUOTED REMARKS : ALSO COMPARE OBSERVED AND COMPUTED PROFILES OF HE I 4026, 4121, 4388, 4438, 4471, 4713, 5016, 5048, 6678 A HE II 4686, 5412 A, MG II 4481 A COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ (A09) PETERS, G.J., POLIDAN, R.S. 1985: CALIBRATION OF FUNDAMENTAL STELLAR QUANTITIES, IAU SYMPOS. 111, D.S.HAYES, A.G.D.PHILIP EDS., P.417 ........................................................................ OBSERV. : OPTICAL DATA FROM (105) HARDORP SCHOLZ 1970: AP.J.S. 19, 193 UV DATA FROM ROGERSON UPSON 1977: AP.J.SUPPL. 35, 37 (COPERNICUS) INSTRUM.: LINELIST: 219 ANALYSIS: LTE(MORTON), T+G(CONT 900..6500 A; PROFILES OF HGAMMA, HDELTA; SI III/IV, S II/III IONIZATION) F-VALUES: WIESE ET AL 1966-69 REMARKS : DETAILS TO BE DISCUSSED ELSEWHERE COMMENTS: CLASS : TGMAA, L? ======================================================================== HD 149414 BD -03 3968 G5V (CN, SUBDWARF, EMISS H+K) AR 16 32.1 DEC -04 07 MV = 9.63 FE/H = --- (R) ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : PG, PORTIONS IN THE RANGE 4600-6600A, 0.28 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: LLWW, LESS THAN 150: ANALYSIS: LTE(ATLAS), T(R-I, V-K), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVES FE/H ONLY COMMENTS: CLASS : DTGMA, (R) ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 5250-6680A, 5.5 A/MM, 0.29 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: 150:, LLWW: PETERSON 1979: ASTROPHYS.J. 235, 491 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 149661 12 OPH K2V (EMISS H+K) AR 16 33.7 DEC -02 13 MV = 5.76 FE/H = 0 (R) ------------------------------------------------------------------------ (246) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 85 ........................................................................ OBSERV. : PG, EGC, 4650-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE LINELIST: LLWW, 200: ANALYSIS: DIFF(SUN), LTE(PEYTREMANN 1974) T(R-I, 102-65) G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUND. ONLY COMMENTS: CF. HEARNSHAW 1976: A.A. 51, 71 CLASS : DTGMA, (R) ======================================================================== HD 150680 ZET HER G0IV (EMISS MG(UV)) AR 16 39.4 DEC +31 42 MV = 2.81 FE/H = 0 I ------------------------------------------------------------------------ ( 37) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1963: ASTROPHYS.J. 138, 97 ........................................................................ OBSERV. : PG, 4000-8700A, 2.8+4.2+6+20.4 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 320: ANALYSIS: COG, DIFF(SUN), EMPIRICAL COG FROM FE I, T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, I ======================================================================== HD 150798 ALF TRA K2II-III (EMISS H+K+MG(UV)) AR 16 43.4 DEC -68 56 MV = 1.92 FE/H = 0 (R) ------------------------------------------------------------------------ (382) KOVACS, N. 1982: ASTRON.ASTROPHYS. 120, 21 ........................................................................ OBSERV. : PG, 4700-6100A, 3.3 A/MM INSTRUM.: ESO 1.5M LINELIST: LLWW, 415 ANALYSIS: DIFF(SUN), LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19 ) T(R-I), G(FEI/II IONIZATION) REMARKS : FINDS LITTLE EVIDENCE FOR NLTE EFFECTS COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 150997 ETA HER G7.5IIIB (EMISS H+K) AR 16 41.2 DEC +39 01 MV = 3.53 FE/H = 0 I ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : COMMENTS: CLASS : (D)A, I ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, I ======================================================================== HD 151680 EPS SCO K2.5III (EMISS H+K+MG(UV)) AR 16 46.9 DEC -34 12 MV = 2.29 FE/H = - (I) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (I) ======================================================================== HD 152792 BD +43 2659 G0V AR 16 52.0 DEC +42 55 MV = 6.74 FE/H = - I ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, I ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA, I ======================================================================== HD 153210 KAP OPH K2III (EMISS H+K+MG(UV)) AR 16 55.3 DEC +09 27 MV = 3.20 FE/H = 0 (R) ------------------------------------------------------------------------ (217) PETERSON, R.C. 1976: ASTROPHYS.J.SUPPL. 30, 61 ........................................................................ OBSERV. : PG, 5190-5890A, 1.7 A/MM INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LLWW, 210: ANALYSIS: LTE(EMPIRICAL), T(EXCITATION FE I, TI I), G(FE I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED, FE I: DIFF(SUN) REMARKS : COMMENTS: CLASS : (D)TGMAA, (R) ======================================================================== HD 154733 HR 6364 K3III (EMISS H+K+MG(UV)) AR 17 04.2 DEC +22 09 MV = 5.56 FE/H = 0 (I) ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA, (I) ======================================================================== HD 155646 BD +00 3654 F6III AR 17 10.3 DEC +00 25 MV = 6.65 FE/H = 0 (R) ------------------------------------------------------------------------ ( 90) ZIELKE, G. 1970: ASTRON.ASTROPHYS. 6, 206 ........................................................................ OBSERV. : PG, 3900-4800A, 10 A/MM; 4800-6700A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LESS THAN 600:, LLWW: ZIELKE 1970: A+A SUPPL. 2, 205 ANALYSIS: LTE(T-TAU SCALED FROM SUN: HOLWEGER 1967: Z.AP. 65, 365), DIFF(HD 136202), T(PROFILES OF HALFA, HBETA, HGAMMA, HDELTA; BVGRI; LINE EXCITATION), G(IONIZATION SI, SC, TI, V, CR, FE, SR), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 155885 36 OPH B K1V (EMISS H+K) AR 17 12.3 DEC -26 32 MV = 5.33 FE/H = 0 (R?) ------------------------------------------------------------------------ (221) PERRIN, M.-N. 1975: ASTRON.ASTROPHYS. 44, 9 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM, 0.3 A INSTRUM.: ESO 1.5M, COUDE LINELIST: 330 ANALYSIS: LTE(PEYTREMANN 1974), DIFF(SUN), T+G(ABS.MAG.+BINARY MASS; R-I, G-I; IONIZATION) ABUNDANCES OF NA, MG FROM LINE PROFILES REMARKS : COMMENTS: CLASS : DTGMAA, (R?) ======================================================================== HD 155886 36 OPH A K0V (EMISS H+K) AR 17 12.3 DEC -26 32 MV = 5.29 FE/H = 0 (R?) ------------------------------------------------------------------------ (221) PERRIN, M.-N. 1975: ASTRON.ASTROPHYS. 44, 9 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM, 0.3 A INSTRUM.: ESO 1.5M, COUDE LINELIST: 330 ANALYSIS: LTE(PEYTREMANN 1974), DIFF(SUN), T+G(ABS.MAG.+BINARY MASS; R-I, G-I; IONIZATION) ABUNDANCES OF NA, MG FROM LINE PROFILES REMARKS : COMMENTS: CLASS : DTGMAA, (R?) ======================================================================== HD 156026 CD -26 12036 K5V (EMISS H+K) AR 17 13.1 DEC -26 29 MV = 6.34 FE/H = 0 R ------------------------------------------------------------------------ (216) STROHBACH, P. 1970: ASTRON.ASTROPHYS. 6, 385 ........................................................................ OBSERV. : PG, 3600-6850A, 10+15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 540: ANALYSIS: LTE(UNBLANKETED), DIFF(SUN), T(B-V, VRI, G-I; WINGS OF HALFA, HBETA; EXCITATION+IONIZATION FE, CR, TI, SC; WIDTHS OF RESONANCE LINES OF NA I, CA I, CR I, AND FE I (MULTIPL. 41..43); STRENGTH OF MGH BAND), G(ABS.MAG.+PARALLAX), REMARKS : COMMENTS: CLASS : DT(G)MAA ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (216) STROHBACH 1970: A+A. 6, 385 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), THEOR. COG FROM LTE MODELS(PEYTREMANN 1970), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 157089 BD +01 3421 F9V AR 17 18.6 DEC +01 29 MV = 6.95 FE/H = -- R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (245) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 71 ........................................................................ OBSERV. : PG, 4500-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, EGC LINELIST: LLWW, 150: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(R-I,I-K), G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUNDANCE ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (292) FOY, R., PROUST, D. 1980: ASTRON.ASTROPHYS. 86, 157 ........................................................................ OBSERV. : DATA FROM ( 3) WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 AND FROM (245) HEARNSHAW 1976: A+A 51, 71 INSTRUM.: LINELIST: ANALYSIS: COG(T-TAU FROM LTE(PEYTREMANN 1974)), DIFF(SUN), T(HEARNSHAW), G(FE I/II IONIZATION), F-VALUES: FOY (1972) REMARKS : COMMENTS: CLASS : DGMA, R ======================================================================== HD 157214 72 HER G0V AR 17 18.8 DEC +32 32 MV = 5.40 FE/H = -- R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 157244 BET ARA K3IB-II (EMISS H+K) AR 17 21.1 DEC -55 29 MV = 2.85 FE/H = + (R) ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5300-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 157881 BD +02 3312 K7V (EMISS H+K) AR 17 23.3 DEC +02 10 MV = 7.54 FE/H = + (R?) ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : PG, ???? , 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH LINELIST: 250 ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, (R?) ======================================================================== HD 157999 SIG OPH K3IAB: (EMISS H+K) AR 17 24.0 DEC +04 11 MV = 4.34 FE/H = 0 (L) ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA, (L) ======================================================================== HD 158614 HR6516 G9IV-V... AR 17 27.8 DEC -01 01 MV = 5.31 FE/H = 0 (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 159181 BET DRA G2IAB: (EMISS H+K+MG(UV)) AR 17 29.3 DEC +52 20 MV = 2.79 FE/H = 0 R ------------------------------------------------------------------------ (277) LUCK, R.E. 1977: ASTROPHYS.J. 218, 752 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MC.DONALD 2.1M, COUDE LINELIST: ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR. COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (423) LUCK, R.E., LAMBERT, D.L. 1981: ASTROPHYS.J. 245, 1018 ........................................................................ OBSERV. : PE, RETICON, 100A SECTIONS CENTERED AT 5380, 6300, 6385, 6425, 6560, 8710A, 0.2A, S/N=100 INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: DOAR, 150-250 ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : T+G FROM LUCK 1977: ASTROPHYS.J. 212, 743 COMMENTS: GIVE ABUNDANCES FOR C, N CLASS : DMSA, R ------------------------------------------------------------------------ (352) FOY, R. 1981: ASTRON.ASTROPHYS. 103, 135 ........................................................................ OBSERV. : DATA FROM LUCK 1977: AP.J. 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T(LUCK), G(IONIZATION FE, TI, CR), F-VALUES: FOY 1972: A+A 18, 26 REMARKS : REANALYIS, GIVE RESULTS ON FE/H ONLY COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 218, 752 INSTRUM.: SEE ALSO: AP.J. 212, 797 LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 160691 MU ARA G3IV-V AR 17 40.2 DEC -51 49 MV = 5.15 FE/H = + (R) ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(SCAN), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 160693 BD +37 2926 G0V AR 17 37.9 DEC +37 13 MV = 8.36 FE/H = -- (I) ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : ONE PLATE ONLY: DATA LESS ACCURATE COMMENTS: CLASS : DTAA, (I) ======================================================================== HD 160762 IOT HER B3IV AR 17 38.0 DEC +46 02 MV = 3.80 FE/H = 0 L ------------------------------------------------------------------------ ( 94) ALLER, L.H., ROSS, J.E. 1967: THE MAGNETIC AND RELATED STARS, R.C.CAMERON ED., MONO BOOK CO., BALTIMORE, P.339 ........................................................................ OBSERV. : PG, 3200-4800A, 2 A/MM; 4800-6600A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: LTE(MIHALAS), EQU.WIDTHS VIA WEIGHTING FUNCTIONS, T(SCAN, COLOURS, IONIZATION), G(BALMER LINE PROFILES), F-VALUES: VARIOUS SOURCES REMARKS : COMMENTS: PRELIMINARY RESULTS CLASS : DTGMAA ------------------------------------------------------------------------ (106) KODAIRA, K., SCHOLZ, M. 1970: ASTRON.ASTROPHYS. 6, 93 ........................................................................ OBSERV. : PG, 3212-6678A, 1+4.3+6.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 240: ANALYSIS: LTE(UNBLANKETED: MIHALAS, STROM+AVRETT), T+G(BJ; IONIZATION SI II/III, S II/III, FE II/III; HGAMMA PROFILE), F-VALUES: VARIOUS SOURCES AS LISTED COMPARE OBS.AND CALC. PROFILES OF HALFA, HDELTA, HE I 4471, 4026, 4388, 4121, 4438, 4713, MG II 4481 A, SCAN 3300-7000 A REMARKS : COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ (104) PETERS, G.J., ALLER, L.H. 1970: ASTROPHYS.J. 159, 525 ........................................................................ OBSERV. : PG, 3400-4770A, 2 A/MM; 4860-6650A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 300: ANALYSIS: LTE(UNBLANKETED: MIHALAS, STROM+AVRETT, BLANKETED: MORTON), T(SCAN+PHOTOMETRY: 1115..7000A), T+G(HALFA..HDELTA PROFILES; IONIZATION SI II/III, S II/III), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ (A09) PETERS, G.J., POLIDAN, R.S. 1985: CALIBRATION OF FUNDAMENTAL STELLAR QUANTITIES, IAU SYMPOS. 111, D.S.HAYES, A.G.D.PHILIP EDS., P.417 ........................................................................ OBSERV. : OPTICAL DATA FROM (104) PETERS ALLER 1970: AP.J. 159, 525 UV DATA FROM UPSON, ROGERSON 1980: AP.J.SUPPL. 42, 175 (COPERNICUS) INSTRUM.: LINELIST: 344 ANALYSIS: LTE(MORTON), T+G(CONT 900..6500 A; PROFILES OF HGAMMA, HDELTA; SI III/IV, S II/III IONIZATION) F-VALUES: WIESE ET AL 1966-69 REMARKS : DETAILS TO BE DISCUSSED ELSEWHERE COMMENTS: CLASS : TGMAA, L ======================================================================== HD 161096 BET OPH K2III (EMISS H+K+MG(UV)) AR 17 41.0 DEC +04 35 MV = 2.77 FE/H = 0 R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 161471 IOT1 SCO F2IAE AR 17 44.0 DEC -40 07 MV = 3.00 FE/H = 0 (R) ------------------------------------------------------------------------ (301) LUCK, R.E. 1979: ASTROPHYS.J. 232, 797 ........................................................................ OBSERV. : PG, 5300-6850A, 9 A/MM INSTRUM.: CTIO 1.5M LINELIST: UP TO 800, DAOR ANALYSIS: LTE(GUSTAFSSON,; RELYEA, KURUCZ), T+G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 161797 MU HER G5IV AR 17 44.5 DEC +27 45 MV = 3.41 FE/H = 0 R ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 161817 BD +25 3344 A2VI (SUBDWARF, HOR.BRANCH) AR 17 44.7 DEC +25 46 MV = 6.97 FE/H = --- R ------------------------------------------------------------------------ ( 38) ALLER, L.H., GREENSTEIN, J.L. 1960: ASTROPHYS.J.SUPPL. 5, 139 ........................................................................ OBSERV. : PG, 3650-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 65: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66), T(SOLAR EXC.TEMP. ASSUMED), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : D(T)AA ------------------------------------------------------------------------ (141) WALLERSTEIN, G., STONE, Y.H., WILLIAMS, J.A. 1962: ASTROPHYS.J. 135, 459 ........................................................................ OBSERV. : DATA FROM ( 38) ALLER, GREENSTEIN 1960: AP.J.SUPPL. 5,139 INSTRUM.: LINELIST: ANALYSIS: COG(FE, TI LINES ONLY), DIFF(ALF CMA), T(B-V) REMARKS : COMMENTS: THIS IS JUST A SHORT APPENDIX CLASS : DTA ------------------------------------------------------------------------ ( 9) KODAIRA, K. 1964: Z.ASTROPHYS. 59, 138 ........................................................................ OBSERV. : PG, 3300-4900A, 10 A/MM; 4900-6700A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 400:, 100: LINES FOR ABUND.ANALYSIS ANALYSIS: LTE, T+G(BJ; CENTRAL INTENSITIES OF HALFA, HGAMMA, MG II K; PROFILES OF HALFA..H8, IONIZATION OF MG I/II, SI I/II, CA I/II, CR I/II, MN I/II, FE I/II), COMPARE OBS.AND CALC. SCAN 3400-11500 A; UVBGRI; PASCHEN JUMP; PROFILES OF H18..H20, MG II 4481, CA I 4227, CA II 3934 A F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMPARE ABUNDANCES WITH SOLAR COMPOSITION (GOLDBERG ET AL. 1960: AP.J.SUPPL. 5, 1 CORRECTED TO THE SAME F-VALUES). COMMENTS: SUPERSEDED BY LATER WORK ( 69) AND (A22) CLASS : (D)TGMAA, R? ------------------------------------------------------------------------ ( 69) KODAIRA, K. 1973: ASTRON.ASTROPHYS. 22, 273 ........................................................................ OBSERV. : DATA FROM ( 9) KODAIRA 1964: Z.ASTROPHYS. 59, 139 INSTRUM.: LINELIST: LW, 43 ANALYSIS: ??? REMARKS : RE-ANALYZES DATA USING NEW F-VALUES COMMENTS: THIS IS MORE A SUMMARY OF RESULTS RATHER THAN A DETAILLED DESCRIPTION OF THE METHODS. THESE METHODS PROBABLY ARE THE SAME AS IN THE PREVIOUS STUDIES. CLASS : TAA ------------------------------------------------------------------------ (379) DANFORD, S.C., LEA, S.M. 1981: ASTRON.J. 86, 1909 ........................................................................ OBSERV. : DATA FROM KODAIRA ET AL.1969: AP.J. 155, 525 INSTRUM.: LINELIST: ANALYSIS: LTE(ATLAS), T+G(CONT: DANFORD 1976: THESIS, YALE UNIV.) F-VALUES: VARIOUS SOURCES (1969-78) LISTED REMARKS : SCALE EQU.WIDTHS TO SCALE OF WRIGHT ET AL.1964, REANALYSIS WITH IMPROVED DAMPING CONSTANTS COMMENTS: CLASS : MAA, R? ------------------------------------------------------------------------ (405) KODAIRA, K., PHILIP, A.G.D. 1981: ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS, IAU COLLOQ. NO.68, A.G.D.PHILIP, D.S.HAYES EDS., L.DAVIS PRESS, SCHENECTADY, N.Y., P. 153 ........................................................................ OBSERV. : ??? 12.5 A/MM ?? INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: ANALYSIS: LTE(ATLAS), T+G(PHOTOMETRY, HDELTA PROFILE) REMARKS : GIVE FE/H ONLY COMMENTS: SUPERSEDED BY (A22) CLASS : TGMA ------------------------------------------------------------------------ (A22) KODAIRA, K., PHILIP, A.G.D. 1984: ASTROPHYS.J. 278, 208 ........................................................................ OBSERV. : PG, 3850-4300A, 12.5 A/MM INSTRUM.: CTIO 4M, CASSEGRAIN, IT LINELIST: LW, 50: ANALYSIS: LTE(ATLAS), DIFF(HD 161817), T+G(B-V, C1, M1, HDELTA WING), F-VALUES: KURUCZ+PEYTREMANN 1975 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 162211 87 HER K2III AR 17 46.8 DEC +25 38 MV = 5.12 FE/H = 0 (R?) ------------------------------------------------------------------------ (325) FOY, R. 1981: ASTRON.ASTROPHYS. 93, 315 ........................................................................ OBSERV. : PG, ??? 6 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FE I/II IONIZATION, R-I, WEAK AND STRONG MG I LINES, WEAK AND STRONG FE I LINES) REMARKS : COMMENTS: CLASS : DTGMAA, (R?) ======================================================================== HD 163428 CD -23 13678 M1IB AR 17 54.1 DEC -23 56 MV = 6.65 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(JOHNSON ET AL.1980: AP.J.SUPPL. 42, 501), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 163588 XI DRA K2III (EMISS H+K) AR 17 52.6 DEC +56 53 MV = 3.75 FE/H = 0 R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 164058 GAM DRA K5III (EMISS H+K) AR 17 55.4 DEC +51 30 MV = 2.23 FE/H = 0 R? ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : PG, ???? , 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH LINELIST: 250 ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, L? ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 165195 BD +03 3579 K3P (EMISS H+K, WEAK METALS) AR 18 02.2 DEC +03 47 MV = 7.32 FE/H = --- R ------------------------------------------------------------------------ ( 14) WALLERSTEIN, G., GREENSTEIN, J.L., PARKER, R., HELFER, H.L., ALLER, L.H. 1963: ASTROPHYS.J. 137, 280 ........................................................................ OBSERV. : PG, 3940-6500A, 8.9+13.5 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN), T(LINE EXCITATION, GRI, IONIZATION) REMARKS : PRELIMINARY ANALYSIS COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM ( 14) WALLERSTEIN ET AL.1963: AP.J. 137, 280 INSTRUM.: LINELIST: USE LINES LONGWARD OF 4300 A ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(G-I), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 6.8 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE, IT LINELIST: 50 ANALYSIS: DIFF(SUN, EPS VIR), COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R? ======================================================================== HD 165341 70 OPH K0V (EMISS H+K) AR 18 02.9 DEC +02 31 MV = 4.03 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 4.5+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: COG(THEOR.COG FROM LTE(PEYTREMANN 1970) MODELS), DIFF(SUN), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (289) PETERSON, R.C. 1978: ASTROPHYS.J. 224, 595 ........................................................................ OBSERV. : PG, 4830-5520A, 1.8 A/MM, 0.07 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE, KRON EGC LINELIST: LW, 90: ANALYSIS: LTE(ATLAS), DIFF(SUN(HSRA)), T(FE I, CO I, NI I EXCITATION), G(CR I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED, FE I/II: DIFF(SUN), REMARKS : TEFF CHECKED WITH R-I COLOUR COMMENTS: CLASS : DTGMAA, L ======================================================================== HD 165760 71 OPH G8III (EMISS H+K) AR 18 04.9 DEC +08 44 MV = 4.64 FE/H = 0 (I) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : DTA, (I) ======================================================================== HD 165908 99 HER F7V (WEAK METALS) AR 18 05.1 DEC +30 33 MV = 5.04 FE/H = - R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 37) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1963: ASTROPHYS.J. 138, 97 ........................................................................ OBSERV. : PG, 4000-4765A, 4 A/MM; 5160-6280A, 6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 320: ANALYSIS: COG, DIFF(SUN), EMPIRICAL COG FROM FE I, T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : DATA FROM ( 3) WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 54) SPITE, M., 1969: ASTRON.ASTROPHYS. 1, 52 ........................................................................ OBSERV. : DATA FROM ( 37) HELFER ET AL.1963: AP.J. 138, 97 PLUS PG, BLUE , 3 A/MM; HBETA 12 A/MM (OHP, COUDE) INSTRUM.: LINELIST: ANALYSIS: LTE(T-TAU SCALED FROM SUN: MUTSCHLECNER 1963), DIFF(SUN), T+G(COG OF FE, CR, TI; ABS.MAG.; HBETA PROFILE) REMARKS : ALSO ANALYZES PROFILES OF NA I D, MG IB LINES (?) COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 166161 BD -08 4566 G5 (WEAK METALS) AR 18 06.9 DEC -08 47 MV = 8.16 FE/H = --- R ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 6.8 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE, IT LINELIST: 50 ANALYSIS: COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), DIFF(SUN, EPS VIR), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 166620 HR 6806 K2V (EMISS H+K) AR 18 08.0 DEC +38 27 MV = 6.37 FE/H = - R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 4.5+6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: COG(THEOR.COG FROM LTE(PEYTREMANN 1970) MODELS), DIFF(SUN), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 168322 HR 6853 G8.5IIIB (EMISS H+K, CN) AR 18 15.5 DEC +40 55 MV = 6.11 FE/H = 0 (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN WEAK, CH SLIGHTLY STRONG? COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 168723 ETA SER K0III-IV (EMISS H+K+MG(UV)) AR 18 18.7 DEC -02 55 MV = 3.26 FE/H = 0 R ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 169414 109 HER K2III (EMISS H+K) AR 18 21.5 DEC +21 45 MV = 3.84 FE/H = - (I) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ======================================================================== HD 170153 KHI DRA A F7V AR 18 22.0 DEC +72 43 MV = 3.57 FE/H = - (R) ------------------------------------------------------------------------ ( 54) SPITE, M., 1967: ANN.ASTROPHYS. 30, 211 ........................................................................ OBSERV. : PG, 4340-6750A, 3.2+4.0 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 700: ANALYSIS: LTE(T-TAU SCALED FROM SUN: MUTSCHLECNER 1963), DIFF(SUN), T+G(COG OF FE, CR, TI; ABS.MAG.+BINARY MASS+EVOL.TRACKS; HBETA PROFILE) ALSO ANALYZES PROFILES OF NA I D, MG IB LINES REMARKS : EQU.WIDTHS ARE CORRECTED FOR THE CONTRIBUTION BY THE SECONDARY STAR. COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 170820 IC 4725 150 G6II AR 18 29.3 DEC -19 10 MV = 7.42 FE/H = 0 L ------------------------------------------------------------------------ ( 12) WALLERSTEIN, G., CONTI, P.S. 1964: ASTROPHYS.J. 140, 858 ........................................................................ OBSERV. : PG, 5000-6600A, 13.5-16.0 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH,LICK 120-INCH, COUDE LINELIST: LLWW, 216 ANALYSIS: COG, DIFF(GAM TAU), T(FE I, TI I EXCITATION, UVBGRI), REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (380) KOMAROV, N.S., SHCHERBAK, A.N. 1980: SOVIET ASTRON. 24, 323 ........................................................................ OBSERV. : DATA FROM ( 12) WALLERSTEIN, CONTI 1964: AP.J. 140, 858 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(ALF BOO), T(FE I EXCITATION), PE(FE I/II IONZATION) REMARKS : COMMENTS: CLASS : DTAA ======================================================================== HD 170886 IC 4725 251 G3II AR 18 29.5 DEC -19 01 MV = 7.01 FE/H = - (L) ------------------------------------------------------------------------ ( 12) WALLERSTEIN, G., CONTI, P.S. 1964: ASTROPHYS.J. 140, 858 ........................................................................ OBSERV. : PG, 5000-6600A, 13.5-16.0 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH,LICK 120-INCH, COUDE LINELIST: LLWW, 216 ANALYSIS: COG, DIFF(GAM TAU), T(FE I, TI I EXCITATION, UVBGRI), REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 171443 ALF SCT K3III (EMISS H+K, CN) AR 18 32.5 DEC -08 17 MV = 3.85 FE/H = 0 (I) ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA, (I) ======================================================================== HD 172167 ALF LYR A0V AR 18 35.2 DEC +38 44 MV = 0.03 FE/H = ? L ------------------------------------------------------------------------ (A01) HUNGER, K. 1955: Z.ASTROPHYS. 36, 42 ........................................................................ OBSERV. : PG, 3350-3900A, 54 A/MM (MCD); 3600-4600A, 2.8 A/MM (MT.W) 3900-5900A, 3.7 A/MM (MCDON. COUDE: HILTNER+WILLIAMS 1949: PHOTOMETRIC ATLAS OF STELLAR SPECTRA, UNIV.MICHIGAN), 4000-4900A, 18 A/MM (LICK) INSTRUM.: MCDONALD 82-INCH, CASSEGRAIN; MT.WILSON 100-INCH, COUDE; LICK 36-INCH, COUDE LINELIST: LLWW, 520: ANALYSIS: LTE(T-TAU ESTIMATED A LA UNSOELD 1942: Z.AP. 21, 229), T(COG, CENTRAL LINE DEPTHS, SCAN 3300..10000A), G(ABS.MAG.+MAIN SEQUENCE), F-VALUES: VARIOUS SOURCES LISTED REMARKS : CONSTANCY OF TOTAL FLUX IS POOR COMMENTS: CLASS : T(G)MAA, L ------------------------------------------------------------------------ (155) HUNGER, K. 1960: Z.ASTROPHYS. 49, 129 ........................................................................ OBSERV. : PG, 4800-8750A, 20.4 A/MM (FROM MATSUSHIMA, GROTH 1960: Z.AP. 49, 126) INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 16 ANALYSIS: LTE(HUNGER 1955: Z.AP. 36, 42 (SLIGHTLY MODIFIED)), COMPARES OBS.AND CALC. PASCHEN 12+13 PROFILES REMARKS : DERIVES N, O, MG, SI, CA ABUNDANCES FROM IR LINES COMMENTS: CLASS : MA ------------------------------------------------------------------------ ( 65) STROM, S.E., STROM, K.M. 1966: ASTRON.J. 71, 181 ........................................................................ OBSERV. : DATA FROM WRIGHT ET AL.1964: PUBL.DOMINION AP.OBS. 12, 173 INSTRUM.: LINELIST: ANALYSIS: LTE(STROM ET AL.1965: ASTRON.J. 70, 148) REMARKS : COMMENTS: SHORT COMMUNICATION CLASS : MAA ------------------------------------------------------------------------ ( 97) STROM, S.E., GINGERICH, O., STROM, K.M. 1966: ASTROPHYS.J. 146, 880 ........................................................................ OBSERV. : DATA FROM (A01) HUNGER 1955: Z.ASTROPHYS. 36, 42 INSTRUM.: LINELIST: LLWW, 350: ANALYSIS: LTE(UNBLANKETED), T+G(UBV, HGAMMA, BJ), F-VALUES: SOURCES INDICATED, BUT NOT REFERENCED REMARKS : COMMENTS: CLASS : TGMAA ------------------------------------------------------------------------ ( 94) ALLER, L.H., ROSS, J.E. 1967: THE MAGNETIC AND RELATED STARS, R.C.CAMERON ED., MONO BOOK CO., BALTIMORE, P.339 ........................................................................ OBSERV. : PG, 3200-4800A, 2 A/MM; 4800-6600A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: LTE(MIHALAS), EQU.WIDTHS VIA WEIGHTING FUNCTIONS, T(SCAN, COLOURS, IONIZATION), G(BALMER LINE PROFILES), F-VALUES: VARIOUS SOURCES REMARKS : COMMENTS: PRELIMINARY RESULTS CLASS : DTGMAA ------------------------------------------------------------------------ ( 70) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 152, 483 ........................................................................ OBSERV. : DATA FROM (A01) HUNGER 1955: Z.ASTROPHYS. 36, 42 INSTRUM.: LINELIST: ANALYSIS: LTE(UNBLANKETED), T(B-V(?), FE I EXCITATION), FE I/II IONIZATION), G(ADOPTED), F-VALUES: CHECKED WITH SUN REMARKS : COMMENTS: CLASS : TMAA ------------------------------------------------------------------------ (117) STROM, S.E., GINGERICH, O., STROM, K.M. 1968: OBSERVATORY 88, 160 ........................................................................ OBSERV. : DATA FROM (A01) HUNGER 1955: Z.ASTROPHYS. 36, 42 INSTRUM.: LINELIST: ANALYSIS: LTE(UNBLANKETED), T(HANBURY BROWN ET AL.1967: MNRAS 137, 393) F-VALUES: WARNER 1967: OBSERVATORY 87, 222 REMARKS : RE-ANALYSIS OF ( 97) WITH DETERMINATION OF MICROTURBULENCE COMMENTS: CLASS : TGMAA ------------------------------------------------------------------------ (107) GEHLICH, U.K. 1969: ASTRON.ASTROPHYS. 3, 169 ........................................................................ OBSERV. : DATA FROM (A01) HUNGER 1955: Z.ASTROPHYS. 36, 42 INSTRUM.: LINELIST: ANALYSIS: LTE(UNBLANKETED, SCHOLZ 1967: Z.AP.65, 243), T+G(SCAN 3300..10000A; HGAMMA, HDELTA PROFILES; IONIZATION), COMPARE OBS.AND CALC.WIDTHS OF HALFA..H8, PASCHEN 12+13 PROFILES, F-VALUES: SOURCES AS LISTED REMARKS : COMMENTS: CLASS : TGMAA ------------------------------------------------------------------------ (124) SMITH, M.A. 1974: ASTROPHYS.J. 189, 101 ........................................................................ OBSERV. : PG, 3860-6260A, 2.7-16 A/MM INSTRUM.: LICK, COUDE LINELIST: LLWW, 160: ANALYSIS: LTE(ATLAS), T(SCHILD ET AL.1971: 166, 95), G(ADOPTED), F-VALUES: CORLISS, WARNER 1971: AP.J.SUPPL. 8, 975 REMARKS : COMMENTS: CLASS : MAA ------------------------------------------------------------------------ (285) BOYARCHUK, A., SNOW, T.P. 1978: ASTROPHYS.J. 219, 515 ........................................................................ OBSERV. : 1330-2950A, 0.1 A INSTRUM.: COPERNICUS LINELIST: LLWW, 420: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 106, 99), T(ASSUMED), F-VALUES: KURUCZ, PEYTREMANN 1975: SAO NO.362 REMARKS : COMMENTS: CLASS : AA ------------------------------------------------------------------------ (321) CASTELLI, F., FARAGGIANA, R. 1979: ASTRON.ASTROPHYS. 79, 174 ........................................................................ OBSERV. : 2000-3000A, 0.4A INSTRUM.: COPERNICUS LINELIST: LW, 90: (ISOLATED LINES) ANALYSIS: COG, LTE(SCHILD ET AL. 1971: AP.J. 166, 95; KPA; ATLAS) REMARKS : COMPARE ABUNDANCE DETERMINATIONS FROM THE VISIBLE AND ULTRAVIOLET, USING VARIOUS MODELS WITH SUITABLE PARAMETERS COMMENTS: CLASS : MAA ------------------------------------------------------------------------ (342) DREILING, L.A., BELL, R.A., 1980: ASTROPHYS.J. 241, 736 ........................................................................ OBSERV. : 4000-5000A, 0.2-0.3 A, S/N= 900 4100-4600A, 0.1-0.15 A, S/N= 600 INSTRUM.: MCDONALD 2.7M, COUDE, RETICON LINELIST: LW, 41 FE I/II, TI II LINES ANALYSIS: LTE(GUSTAFSSON, WITH HE I OPACITY ADDED), NLTE(MIHALAS), T+G(4 COMBINATIONS), COMPARE OBS.AND CALC. ABSOLUTE FLUXES AT 5556, 10400 A; FLUX DISTRIBUTION 3300..10800 A; PROFILES OF HALFA..HGAMMA, PASCHEN 13..15, BRACKETT LINES; COG OF FE I, II, TI II, F-VALUES: FE I: LABORATORY, FE II: DIFF(SUN, HSRA) REMARKS : COMPUTE SYNTHETIC SPECTRUM FOR 1200..3000 A COMMENTS: DERIVATION OF ABUNDANCES WAS NOT PRIMARY AIM OF WORK CLASS : (TG)MN(S)(A), L ------------------------------------------------------------------------ (389) SADAKANE, K., NISHIMURA, M. 1981: PUBL.ASTRON.SOC.JAPAN 33, 189 ........................................................................ OBSERV. : PG, 3250-3640A, 4 A/MM INSTRUM.: OKAYAMA OBS. 1.9M, COUDE LINELIST: LW, 60 UNBLENDED LINES ANALYSIS: LTE(ATLAS), T(CODE ET AL.1976: AP.J. 203, 417), G(CODE 1975: DUDLEY OBS.REPT. 9, 221), F-VALUES: KURUCZ, PEYTREMANN 1975 REMARKS : COMPARE ABUNDANCES DERIVED FROM REGION 3900-4900A (CF. (395) SADAKANE, NISHIMURA 1979: PASJ 31, 189) WITH THOSE DERIVED FROM NEAR UV LINES: FIND METAL DEFICIENCY. COMMENTS: CLASS : MAA, L ======================================================================== HD 172365 HR 7008 F8IB-II AR 18 37.1 DEC +05 13 MV = 6.38 FE/H = -- (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 174947 33 SGR K0IAB: AR 18 51.0 DEC -21 25 MV = 5.69 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 174959 HR 7115 B6IV AR 18 49.8 DEC +36 29 MV = 6.08 FE/H = -- (L) ------------------------------------------------------------------------ (331) HEACOX, W.D. 1979: ASTROPHYS.J.SUPPL. 41, 675 ........................................................................ OBSERV. : PG, 3100-4700A, 6.8 A/MM, 0.14 A, MN III (1285 A) INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LLWW, 80: ANALYSIS: LTE(KPA), T(C0,M0), G(HGAMMA, HDELTA) FE F-VALUES OF WARNER(1967), CORRECTED AFTER SMITH(1976) REMARKS : GIVES ABUNDANCES FOR XI = 0 AND 3 KM/S COMMENTS: CLASS : TGMAA, (L) ======================================================================== HD 174974 NU1 SGR K2IAB: (EMISS H+K) AR 18 51.1 DEC -22 48 MV = 4.83 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 175305 BD +74 792 G5III (WEAK METALS, SUBDWARF) AR 18 48.5 DEC +74 40 MV = 7.20 FE/H = --- (R) ------------------------------------------------------------------------ (335) WALLERSTEIN, G., PILACHOWSKI, C., GEREND, D., BAIRD, S., CANTERNA, R. 1979: MONTHLY NOTICES ROY.ASTRON.SOC. 186, 691 ........................................................................ OBSERV. : PG, 3700-6300A, 8.9+13.5 A/MM; 6250-6350A, 6.4 A/MM (KPNO) INSTRUM.: MT.PALOMAR 200-INCH, COUDE; KPNO 4M, ECHELLE LINELIST: LLWW, 210: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T(UBVKT1T2), G(FE I/II, CR I/II, TI I /II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 175329 OMG PAV K2IIICNVAR... AR 18 54.2 DEC -60 16 MV = 5.10 FE/H = -- (R) ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(IR NARROW BAND INDEX), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 179761 21 AQL B8II-III AR 19 11.2 DEC +02 16 MV = 5.15 FE/H = 0 R ------------------------------------------------------------------------ (190) SEARLE, L., LUNGERSHAUSEN, W., SARGENT, W.L.W. 1966: ASTROPHYS.J. 145, 141 ........................................................................ OBSERV. : PG, 3200-3600A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 29 ANALYSIS: COG, DIFF(OMI PEG), THEOR.COG FROM WRUBEL 1949 T(TI II EXCITATION), F-VALUES: CORLISS, BOZMAN 1962 REMARKS : FIND ABUNDANCES OF FE, CR, MN, TI TO BE NORMAL COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (A25) ADELMAN, S.J. 1984: MONTHLY NOTICES ROY.ASTRON.SOC. 206, 637 ........................................................................ OBSERV. : PG, ??? , 4-6.7 A/MM INSTRUM.: MT.WILSON, MT.PALOMAR, LICK LINELIST: 100:, LW: MICROFICHE MN 206/1 ANALYSIS: LTE(ATLAS), DIFF(SUN), T+G(SCAN 3300-7100A, HGAMMA PROFILE), F-VALUES: BLACKWELL, KORNBLITH+BRIDGES, AND OTHERS REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 180028 BD +05 4087 F6IB AR 19 12.3 DEC +05 58 MV = 6.97 FE/H = - (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 180262 HR 7300 G8II-III (EMISS H+K, CH) AR 19 13.0 DEC +15 00 MV = 5.57 FE/H = 0 (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN, CH STRONG COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 180711 DEL DRA G9III (EMISS H+K+MG(UV)) AR 19 12.5 DEC +67 34 MV = 3.07 FE/H = 0 R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 3954-4822A, 2 A/MM; 5325-6635A, 3 A/MM INSTRUM.: DAO 48-INCH, COUDE LINELIST: 800:, LLWW: KOELBLOED,VAN PARADIJS 1975: A+A SUPPL. 19, 101 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 180809 TET LYR K0II (EMISS H+K) AR 19 14.6 DEC +38 03 MV = 4.36 FE/H = 0 (R) ------------------------------------------------------------------------ (254) PILACHOWSKI, C.A. 1977: ASTRON.ASTROPHYS. 54, 465 ........................................................................ OBSERV. : PG, ??? , 3.4-10 A/MM INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LW: TO BE PUBLISHED ??? ANALYSIS: LTE(CARBON, GINGERICH 1969), DIFF(EPS VIR), T(CONT.SLOPE 5400/6300A), G(MG II B LINE PROFILES, FE I/II, TI I/II, CR I/II IONIZATION), F-VALUES: VARIOUS SOURCES REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 181276 KAP CYG G9III (EMISS H+K) AR 19 15.9 DEC +53 17 MV = 3.80 FE/H = 0 L ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T+G(THEOR./EMPIR. COG) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, L ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 181470 HR 7338 A0III AR 19 17.3 DEC +37 21 MV = 6.22 FE/H = -- R ------------------------------------------------------------------------ (331) HEACOX, W.D. 1979: ASTROPHYS.J.SUPPL. 41, 675 ........................................................................ OBSERV. : PG, 3100-4700A, 6.8 A/MM, 0.14 A, MN III (1285 A) INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LLWW, 80: ANALYSIS: LTE(KPA), T(C0,M0), G(HGAMMA, HDELTA) FE F-VALUES OF WARNER(1967), CORRECTED AFTER SMITH(1976) REMARKS : GIVES ABUNDANCES FOR XI = 0 AND 3 KM/S COMMENTS: STAR IS USED AS REFERENCE FOR HG-MN STARS CLASS : TGMAA ------------------------------------------------------------------------ (394) SADAKANE, K. 1981: PUBL.ASTRON.SOC.PACIFIC 93, 587 ........................................................................ OBSERV. : PG, 3850-4640A, 2.3 A/MM INSTRUM.: DAO LINELIST: LLWW, 150: ANALYSIS: LTE(ATLAS), T+G(B-V, B-Y, BETA; HGAMMA PROFILE; FE I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : TGMAA, R ======================================================================== HD 182274 BD +19 3996 F6V AR 19 21.0 DEC +19 17 MV = 7.81 FE/H = - (R) ------------------------------------------------------------------------ (A30) LUCK, R.E., BOND, H.E. 1982: ASTROPHYS.J. 259, 792 ........................................................................ OBSERV. : PG, 3800-5000A, 9 A/MM; 50A SECTIONS IN 5100-7800A, 0.2A, S/N= 30..50 (RETICON) INSTRUM.: MT.WILSON 100-INCH, COUDE, RETICON, MT.PALOMAR 200-INCH LINELIST: 200 OR MORE ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 182572 31 AQL G8IV... AR 19 22.6 DEC +11 50 MV = 5.16 FE/H = + R ------------------------------------------------------------------------ ( 87) HEARNSHAW J.B. 1971: ASTROPHYS.J. 168, 109 ........................................................................ OBSERV. : PG, 4468-4923A, 10.2 A/MM; 5497-6810A, 6.7 A/MM INSTRUM.: MT.STROMLO 74-INCH, COUDE LINELIST: 372 ANALYSIS: COG(WRUBEL 1949), DIFF(SUN), T(SCAN 3862..7550A, R-I, HALFA PROFILE) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I, SCAN), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (246) HEARNSHAW, J.B. 1976: ASTRON.ASTROPHYS. 51, 85 ........................................................................ OBSERV. : PG, EGC, 4650-5600A, 4 A/MM, 0.1 A INSTRUM.: SAO 1.5M, CASSEGRAIN, ECHELLE LINELIST: LLWW, 200: ANALYSIS: DIFF(SUN), LTE(PEYTREMANN 1974) T(R-I, SCAN 3200-10870A(HEARNSHAW 1971)) G(FE I/II IONIZATION) REMARKS : DERIVES FE ABUND. ONLY, COMPARISON WITH NO.(208): DISCREPANCY BETWEEN SPECTROCOPIC AND TRIGONOMETRIC PARALLAX SEEMS JUST SIGNIFICANT COMMENTS: CF. HEARNSHAW 1976: A.A. 51, 71 CLASS : DTGMA, R ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 INSTRUM.: LINELIST: 13 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(PREVIOUS WORK.....), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : TMA, R ======================================================================== HD 184266 BD -16 5359 G0 (WEAK METALS) AR 19 31.4 DEC -16 25 MV = 7.57 FE/H = --- (R) ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 184406 MU AQL K3IIIB (EMISS H+K) AR 19 31.6 DEC +07 16 MV = 4.45 FE/H = 0 R? ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 43) HELFER 1968: AP.J.SUPPL. 16, 1 INSTRUM.: LINELIST: ANALYSIS: DIFF(MEAN OF: GAM TAU, DEL TAU, EPS TAU, EPS VIR), LTE(ALTAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ======================================================================== HD 184499 BD +32 3474 G0V AR 19 31.6 DEC +33 05 MV = 6.61 FE/H = -- R ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3800-4700A, 13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (309) PETERSON, R.C. 1980: ASTROPHYS.J. 235, 491 ........................................................................ OBSERV. : PG, PORTIONS IN THE RANGE 4600-6600A, 0.28 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: LLWW, LESS THAN 150: ANALYSIS: LTE(ATLAS), T(R-I, V-K), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVES FE/H ONLY COMMENTS: CLASS : DTGMA, R ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : PG, 5250-6680A, 5.5 A/MM, 0.29 A INSTRUM.: KPNO 4M, ECHELLE, IT LINELIST: 150:, LLWW: PETERSON 1980: ASTROPHYS.J. 235, 491 ANALYSIS: LTE(ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 184711 CD -40 13389 G0 (WEAK METALS) AR 19 33.8 DEC -39 51 MV = 7.99 FE/H = ---- R ------------------------------------------------------------------------ (280) SPITE, M., SPITE, F. 1978: ASTRON.ASTROPHYS. 67, 23 ........................................................................ OBSERV. : DATA FROM (328) SPITE SPITE 1979, A+A 76, 150 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(R-I), G(IONIZATION FE, TI, CR) REMARKS : COMMENTS: CLASS : DTGMA ------------------------------------------------------------------------ (328) SPITE, M., SPITE, F. 1979: ASTRON.ASTROPHYS. 76, 150 ........................................................................ OBSERV. : PG, 4320-4950A, 5800-6330A, 12 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LLWW, 240: ANALYSIS: LTE(GUSTAFSSON), DIFF(HD 122563, SUN) T(R-I, HBETA, HGAMMA), G(IONIZATION FE, TI, CR) REMARKS : TAKE INTO ACCOUNT VARIATION OF COG WITH EACH IONIC SPECIES: SOME IMPORTANCE FOR NA, MG, BA, Y COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (322) SPITE, M., SPITE, F. 1980: ASTRON.ASTROPHYS. 89, 118 ........................................................................ OBSERV. : PG, 3930-3970A, 7.1 A/MM INSTRUM.: ESO 1.5M, COUDE, ECHELLE, LALLEMAND EGC LINELIST: LW, 4 ANALYSIS: LTE(PEYTREMANN 1974, GUSTAFSSON), DIFF(SUN), T+G(SPITE'S 1979: A+A 76, 150), F-VALUES: WIESE 1969 NSRDS-NBS 22 SPECTRUM SYNTHESIS REMARKS : DERIVE AL ABUNDANCE ONLY COMMENTS: FE AND MG ABUNDANCES ARE QUOTED FROM OTHER WORKS CLASS : DMSA ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 6.8 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE, IT LINELIST: 50 ANALYSIS: DIFF(SUN, EPS VIR), COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : DATA FROM (328) SPITE SPITE 1979, A+A 76, 150 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(SPITE), SOLAR F-VALUES REMARKS : REANALYSIS COMMENTS: CLASS : DMAA, R ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-6800A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 185144 SIG DRA K0V (EMISS H+K) AR 19 32.5 DEC +69 35 MV = 4.70 FE/H = 0 R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 6000?-6500?A, 6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I) G(TRIG. PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DTMA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 185622 HR 7475 K4IB AR 19 37.2 DEC +16 27 MV = 6.38 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(JOHNSON ET AL.1980: AP.J.SUPPL. 42, 501), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 185657 HR 7477 G6V AR 19 36.5 DEC +49 10 MV = 6.47 FE/H = - (L) ------------------------------------------------------------------------ ( 5) PAGEL, B.E.J. 1964: ROY.OBS.BULL. 87 ........................................................................ OBSERV. : PG, 3700-4900A, 9 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG, DIFF(SUN), T(EMPIR. COG FROM FE I LINES) REMARKS : RGI COLOURS ARE USED AS A CHECK ON THE DERIVED TEMPERATURES COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 186408 16 CYG A G1.5VB AR 19 40.5 DEC +50 25 MV = 5.96 FE/H = 0 R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (327) PERRIN, M.-N., SPITE, M. 1981: ASTRON.ASTROPHYS. 94, 207 ........................................................................ OBSERV. : PG, 4360-5940A, 12 A/MM INSTRUM.: OHP 1.5+1.9M, COUDE LINELIST: LLWW, 300: ANALYSIS: LTE(PEYTREMANN 1974), DIFF(SUN), T(HBETA, HGAMMA PROFILES) G(FE I/II, TI I/II, CR I/II IONIZATION) COMPARE OBS.AND CALC. COLOURS B-V, R-I, V-L, ... REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 186427 16 CYG B G3V AR 19 40.5 DEC +50 24 MV = 6.20 FE/H = 0 R ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 135 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (323) BRANCH, D., LAMBERT, D.L., TOMKIN, J. 1980: ASTROPHYS.J. 241, L87 ........................................................................ OBSERV. : 100A WIDE REGIONS AT 6578, 6752A, 0.2 A, S/N= 300 INSTRUM.: MCDONALD 2.7M, COUDE, RETICON LINELIST: LW, 21 FE I LINES ANALYSIS: LTE(T-TAU SCALED FROM SUN(HOLWEGER, MUELLER 1974)), DIFF(SUN), T(HALFA PROFILE, LTE(ATLAS)), G(ASSUMED) REMARKS : COMMENTS: CLASS : DTAA, R ------------------------------------------------------------------------ (327) PERRIN, M.-N., SPITE, M. 1981: ASTRON.ASTROPHYS. 94, 207 ........................................................................ OBSERV. : PG, 4360-5940A, 12 A/MM INSTRUM.: OHP 1.5+1.9M, COUDE LINELIST: LLWW, 300: ANALYSIS: LTE(PEYTREMANN 1974), DIFF(SUN), T(HBETA, HGAMMA PROFILES) G(FE I/II, TI I/II, CR I/II IONIZATION) COMPARE OBS.AND CALC. COLOURS B-V, R-I, V-L, ... REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 186791 GAM AQL K3II (EMISS H+K+MG(UV)) AR 19 43.9 DEC +10 29 MV = 2.72 FE/H = 0 (I) ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA, (I) ======================================================================== HD 187238 BD +22 3812 K3IAB-B AR 19 46.0 DEC +22 38 MV = 7.7 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 187299 BD +24 3889 G5IAB-B AR 19 46.3 DEC +24 53 MV = 7.12 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 187691 OMI AQL F8V AR 19 48.6 DEC +10 17 MV = 5.10 FE/H = 0 R ------------------------------------------------------------------------ (317) GEHREN, T. 1979: ASTRON.ASTROPHYS. 75, 73 ........................................................................ OBSERV. : PG, 4400-6820A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 480:, LLWW: GEHREN ET AL.1978: A+A SUPPL. 31, 297 ANALYSIS: LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), T(LINE PROFILES OF HALFA, HGAMMA), G(IONIZATION SI, TI, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (317) GEHREN 1979: A+A 75, 73 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ======================================================================== HD 187923 HR 7569 G0V AR 19 49.7 DEC +11 30 MV = 6.10 FE/H = 0 L ------------------------------------------------------------------------ ( 31) WALLERSTEIN, G., HELFER, H.L. 1961: ASTROPHYS.J. 133, 562 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 120:, LLWW: ( 29) HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE( IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, LLWW: HELFER ET AL. 1960: AP.J. 132, 553 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ======================================================================== HD 188056 20 CYG K3III (EMISS H+K, CN) AR 19 49.4 DEC +52 52 MV = 5.03 FE/H = 0 L ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6700A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (138) STROM, S.E., STROM, K.M., CARBON, D.F. 1971: ASTRON.ASTROPHYS. 12, 177 ........................................................................ OBSERV. : DATA FROM ( 43) HELFER 1968: AP.J.SUPPL. 16, 1 INSTRUM.: LINELIST: ANALYSIS: DIFF(MEAN OF: GAM TAU, DEL TAU, EPS TAU, EPS VIR), LTE(ALTAS; CARBON, GINGERICH), T(HLJ; FE I, TI I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, L ======================================================================== HD 188119 EPS DRA G8III (EMISS H+K) AR 19 48.4 DEC +70 08 MV = 3.83 FE/H = - (L?) ------------------------------------------------------------------------ (248) VAN PARADIJS, J., KESTER, D. 1976: ASTRON.ASTROPHYS. 53, 1 ........................................................................ OBSERV. : PG, 4394-4822A, 2 A/MM; 5325-6635A, 3 A/MM INSTRUM.: DAO 48-INCH, COUDE LINELIST: 800:, LLWW: KOELBLOED,VAN PARADIJS 1975: A+A SUPPL. 19, 101 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: DERIVE C, N, O ABUNDANCES ONLY, AND JUST REPORT FE/H VALUE CLASS : DTGMA, (L?) ======================================================================== HD 188510 BD +10 4091 G5VWE (WEAK METALS) AR 19 52.8 DEC +10 36 MV = 8.82 FE/H = --- (L) ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, (L) ======================================================================== HD 188512 BET AQL G8IV (EMISS H+K) AR 19 52.8 DEC +06 17 MV = 3.71 FE/H = 0 R ------------------------------------------------------------------------ (184) BACJAR, R. 1969: CONTR.ASTRON.OBS.SKALNATE PLESO 4, 63 ........................................................................ OBSERV. : PG, 3300-4800A, 9+18 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66 T(LINE EXCITATION), PE(IONIZATION TI, V, SC, Y), F-VALUES: CORLISS, BOZMAN 1962 CHECKED WITH SOLAR SPECTRUM REMARKS : COMMENTS: CLASS : (D)TAA ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T+G(THEOR./EMPIR. COG) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 188947 ETA CYG K0III (EMISS H+K) AR 19 54.4 DEC +34 57 MV = 3.89 FE/H = 0 R ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T+G(THEOR./EMPIR. COG) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 189567 HR7644 G3V AR 20 00.5 DEC -67 27 MV = 6.07 FE/H = - (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 190178 CD -28 16387 F3V (WEAK METALS) AR 20 01.7 DEC -28 25 MV = 9.55 FE/H = --- (L) ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, (L) ======================================================================== HD 190248 DEL PAV G7IV AR 20 03.8 DEC -66 19 MV = 3.56 FE/H = + R ------------------------------------------------------------------------ (113) RODGERS, A.W. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 145, 151 ........................................................................ OBSERV. : PG, 5600-6800A, 2.6 A/MM INSTRUM.: MT.STROMLO 74-INCH, COUDE LINELIST: LLWW, 300: ANALYSIS: COG(WRUBEL 1949), DIFF(SUN), T(HALFA PROFILE CALC.FROM GREY ATMOSPHERE; SCAN 3300-12000A, LTE(MIHALAS 1964); R-I, B-V; FE I EXCITATION), F-VALUES: CORLISS, WARNER 1964 REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (135) HARMER, D.L., PAGEL, B.E.J., POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 150, 409 ........................................................................ OBSERV. : PG, 4200-5000A, 6.7 A/MM; 5300-6710A, 10 A/MM INSTRUM.: MT.STROMLO 74-INCH, COUDE LINELIST: 167 ANALYSIS: COG(VAN DER HELD SHAPE), DIFF(SUN), T(FE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, R ======================================================================== HD 190287 CD -35 13902 G6VW (WEAK METALS) AR 20 02.4 DEC -35 04 MV = 8.54 FE/H = --- (R) ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 190323 BD +14 4158 G0IA AR 20 01.5 DEC +14 50 MV = 6.86 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 190360 HR 7670 G6IV+... AR 20 01.6 DEC +29 46 MV = 5.71 FE/H = 0 (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 190404 BD +22 3908 K1V AR 20 01.8 DEC +23 13 MV = 7.28 FE/H = 0 R ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : PG, 4400-6800A, 9.7+12.4 A/MM, 0.3A INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : COMMENTS: PROBABLY SUPERSEDED BY (224) CLASS : DTGMAA, L ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : DATA FROM ( 41) CAYREL DE STROBEL 1966: ANN.ASTR. 29, 413 INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY REF.(41) DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ (216) STROHBACH, P. 1970: ASTRON.ASTROPHYS. 6, 385 ........................................................................ OBSERV. : DATA FROM ( 41) CAYREL DE STROBEL 1966: ANN.ASTR. 29, 413 INSTRUM.: LINELIST: ANALYSIS: LTE(UNBLANKETED), DIFF(SUN), T(B-V, VRI, G-I; WINGS OF HALFA, HBETA; EXCITATION+IONIZATION FE, CR, TI, SC; WIDTHS OF RESONANCE LINES OF NA I, CA I, CR I, AND FE I (MULTIPL. 41..43); STRENGTH OF MGH BAND), G(ABS.MAG.+PARALLAX), REMARKS : COMMENTS: CLASS : DT(G)MAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM ( 41) CAYREL 1966: ANN.ASTROPHYS. 29, 413 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), THEOR. COG FROM LTE MODELS(PEYTREMANN 1970), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 191046 BD +35 3962 K0III AR 20 04.6 DEC +36 05 MV = 7.03 FE/H = - (I) ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN WEAK COMMENTS: CLASS : (D)A, (I) ======================================================================== HD 191408 HR 7703 K3V (EMISS H+K) AR 20 07.9 DEC -36 14 MV = 5.31 FE/H = 0 (R) ------------------------------------------------------------------------ (221) PERRIN, M.-N. 1975: ASTRON.ASTROPHYS. 44, 9 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM, 0.3 A INSTRUM.: ESO 1.5M, COUDE LINELIST: 330 ANALYSIS: LTE(PEYTREMANN 1974), DIFF(SUN), T+G(ABS.MAG.+ASSUMED MASS; R-I, G-I; IONIZATION) ABUNDANCES OF NA, MG FROM LINE PROFILES REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 191692 TET AQL B9.5III AR 20 08.7 DEC -00 58 MV = 3.23 FE/H = 0 (R) ------------------------------------------------------------------------ (354) ADELMAN, S.J., NASSON, M.A. 1980: PUBL.ASTRON.SOC.PACIFIC 92, 346 ........................................................................ OBSERV. : PG, 3300-7100A, 4.3+8.9 A/MM INSTRUM.: MT.WILSON 100-INCH, KPNO 4M, COUDE LINELIST: LLWW, 200: ANALYSIS: LTE(ATLAS), T(SCAN 3300-7100A), G(HGAMMA PROFILE), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMPARE ABUNDANCES WITH SOLAR ONES THAT HAD BEEN DERIVED WITH THE SAME F-VALUES COMMENTS: CLASS : TGMAA, (R) ======================================================================== HD 192310 HR 7722 K0V VAR (EMISS H+K) AR 20 12.2 DEC -27 11 MV = 5.73 FE/H = 0 R ------------------------------------------------------------------------ (216) STROHBACH, P. 1970: ASTRON.ASTROPHYS. 6, 385 ........................................................................ OBSERV. : PG, 3600-6850A, 10+15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 540: ANALYSIS: LTE(UNBLANKETED), DIFF(SUN), T(B-V, VRI, G-I; WINGS OF HALFA, HBETA; EXCITATION+IONIZATION FE, CR, TI, SC; WIDTHS OF RESONANCE LINES OF NA I, CA I, CR I, AND FE I (MULTIPL. 41..43); STRENGTH OF MGH BAND), G(ABS.MAG.+PARALLAX), REMARKS : COMMENTS: CLASS : DT(G)MAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (216) STROHBACH 1970: A+A 6, 385 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), THEOR. COG FROM LTE MODELS(PEYTREMANN 1970), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 192577 31 CYG K2II+... (EMISS H+K) AR 20 12.0 DEC +46 35 MV = 3.79 FE/H = 0 R ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 192947 ALF2 CAP G9III (EMISS H+K) AR 20 15.3 DEC -12 42 MV = 3.57 FE/H = 0 R ------------------------------------------------------------------------ (286) FOY, R. 1978: ASTRON.ASTROPHYS. 67, 311 ........................................................................ OBSERV. : PG, ??? , 12.4 A/MM INSTRUM.: ESO LINELIST: TO BE PUBLISHED ANALYSIS: COG( LTE(PEYTREMANN 1974)), T(R-I), G(FE I /II IONIZATION), F-VALUES AS COMPILED BY FOY 1972: A+A 18, 26 AND BY CAYREL ET AL. 1977: A+A 54, 797 REMARKS : STUDIES MICROTURBULENCE COMMENTS: ONLY FE/H ABUNDANCE DERIVED CLASS : (D)TGMA, R ------------------------------------------------------------------------ (325) FOY, R. 1981: ASTRON.ASTROPHYS. 93, 315 ........................................................................ OBSERV. : PG, ??? 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FE I/II IONIZATION, R-I, WEAK AND STRONG MG I LINES, WEAK AND STRONG FE I LINES) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 193432 NU CAP B9.5V AR 20 17.9 DEC -12 55 MV = 4.76 FE/H = ? R ------------------------------------------------------------------------ (190) SEARLE, L., LUNGERSHAUSEN, W., SARGENT, W.L.W. 1966: ASTROPHYS.J. 145, 141 ........................................................................ OBSERV. : PG, 3200-3600A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 29 ANALYSIS: COG, DIFF(OMI PEG), THEOR.COG FROM WRUBEL 1949 T(TI II EXCITATION), F-VALUES: CORLISS, BOZMAN 1962 REMARKS : DERIVE ABUNDANCES OF FE, CR, MN, TI COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (374) WOLFF, S.C. 1970: ASTROPHYS.J.SUPPL. 15, 21 ........................................................................ OBSERV. : PG, 3860-4620A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LW, 22 SELECTED UNBLENDED LINES ANALYSIS: COG(WRUBEL 1949), T(SCAN 4000-8800A, LTE(MIHALAS 1966)), G(HGAMMA PROFILES, LTE(MIHALAS 1966)), F-VALUES: WARNER 1967, CORLISS, BOZMAN 1962 REMARKS : USES ONLY ONE OR TWO LINES PER ION, MOST OF WHICH LIE ON THE COG'S FLAT PORTION. COMMENTS: THIS STAR SERVES AS STANDARD FOR STUDY OF AP STARS CLASS : TG(M)A ------------------------------------------------------------------------ (197) CONTI, P.S. 1970: ASTRON.ASTROPHYS. 7, 213 ........................................................................ OBSERV. : PG, 3850-4700, 4 A/MM INSTRUM.: LICK 120-INCH LINELIST: LW, 60: ANALYSIS: COG(COWLEY+COWLEY 1964 SHAPE), DIFF(HD 73666), T(HGAMMA PROFILE, B-V), G(ADOPTED) REMARKS : COMMENTS: CLASS : D(T)AA, L ------------------------------------------------------------------------ (110) ADELMAN, S.J. 1973: ASTROPHYS.J. 182, 531 ........................................................................ OBSERV. : PG, , 4.5+6.7+10.4 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: LTE(ATLAS), T(SCAN 3500-8800A), G(HGAMMA PROFILE), F-VALUES: VARIOUS SOURCES AS LISTED, REMARKS : COMMENTS: NOTE THAT SOLAR ABUNDANCES GIVEN HERE ARE QUITE DIFFERENT FROM THE (MORE CAREFULLY SELECTED) VALUES USED IN THE LATER PAPER (354) ADELMAN, NASSON 1980: PASP 92, 346 CLASS : TGMAA ------------------------------------------------------------------------ (142) ADELMAN, S.J. 1973: ASTROPHYS.J. 183, 95 ........................................................................ OBSERV. : PG, 3850-3870A, 3968-4650A, 4.5 A/MM INSTRUM.: LICK, MT.PALOMAR 200-INCH, COUDE LINELIST: ANALYSIS: COG(LTE(ATLAS)), T(SCAN), G(HGAMMA PROFILE) REMARKS : COMMENTS: CLASS : TGMAA ------------------------------------------------------------------------ (265) ALLEN, M.S. 1977: ASTROPHYS.J. 213, 121 ........................................................................ OBSERV. : PG, 3700-4150A, 4200-4650A, 2.4 A/MM, 0.074A (FWHM) INSTRUM.: DAO 1.2M, COUDE, IMAGE SLICER LINELIST: 66, DAOR ANALYSIS: LTE(KCP 1969), T+G(UBV, HGAMMA, FE I/II IONIZATION) F-VALUES: EXPERIMENTAL, THEORETICAL, SOLAR REMARKS : DERIVES ABUNDANCES FOR FE, SR, Y ONLY COMMENTS: USES STAR AS COMPARISON FOR HG-MN STARS CLASS : (D)TGMA ------------------------------------------------------------------------ (274) ALLEN, M.S., COWLEY, C.R. 1977: PUBL.ASTRON.SOC.PACIFIC 89, 386 ........................................................................ OBSERV. : DATA FROM (110) ADELMAN 1973: AP.J. 182, 531 INSTRUM.: LINELIST: ANALYSIS: LTE(KCP 1969), T+G(FROM (265) ALLEN 1977: AP.J. 213, 121), F-VALUES: AS DISCUSSED REMARKS : DERIVE ABUNDANCES FOR CR, FE ONLY COMMENTS: CLASS : MA ------------------------------------------------------------------------ (331) HEACOX, W.D. 1979: ASTROPHYS.J.SUPPL. 41, 675 ........................................................................ OBSERV. : PG, 3100-4700A, 6.8 A/MM, 0.14 A, MN III (1285 A) INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LLWW, 80: ANALYSIS: LTE(KPA), T(C0,M0), G(HGAMMA, HDELTA) FE F-VALUES OF WARNER(1967), CORRECTED AFTER SMITH(1976) REMARKS : GIVES ABUNDANCES FOR XI = 0 AND 3 KM/S COMMENTS: USES STAR AS COMPARISON FOR HG-MN STARS CLASS : TGMAA ------------------------------------------------------------------------ (354) ADELMAN, S.J., NASSON, M.A. 1980: PUBL.ASTRON.SOC.PACIFIC 92, 346 ........................................................................ OBSERV. : DATA FROM (110) ADELMAN 1973: AP.J. 182, 531 INSTRUM.: LINELIST: LLWW, 200: ANALYSIS: LTE(ATLAS), T(SCAN 3300-7100A), G(HGAMMA PROFILE), F-VALUES: VARIOUS SOURCES AS LISTED, APPLY NLTE CORRECTION FOR O I REMARKS : COMPARE ABUNDANCES WITH SOLAR ONES THAT HAD BEEN DERIVED WITH THE SAME F-VALUES COMMENTS: CLASS : (D)TGMAA, R ------------------------------------------------------------------------ (A25) ADELMAN, S.J. 1984: MONTHLY NOTICES ROY.ASTRON.SOC. 206, 637 ........................................................................ OBSERV. : DATA FROM (110) ADELMAN 1973: AP.J. 182, 531 INSTRUM.: LINELIST: 190: ANALYSIS: LTE(ATLAS), DIFF(SUN), T+G(SCAN 3300-7100A, HGAMMA PROFILE), F-VALUES: BLACKWELL, KORNBLITH+BRIDGES, AND OTHERS REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 193664 HR 7783 G3V AR 20 17.0 DEC +66 41 MV = 5.93 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(TRIG.PARALL.+EVOL.TRACKS), FE+CH: DIFF(SUN) REMARKS : EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 194093 GAM CYG F8IAB: (EMISS MG(UV)) AR 20 20.4 DEC +40 06 MV = 2.20 FE/H = 0 R ------------------------------------------------------------------------ (167) WRIGHT, K.O. 1951: PUBL.DOM.ASTROPHYS.OBS.VICTORIA 8, 1 ........................................................................ OBSERV. : PG, 3700-6750A, 4.8...20.8 A/MM INSTRUM.: DAO 72-INCH, CASSEGRAIN LINELIST: LLWW, 800 ANALYSIS: COG, DIFF(SUN), THEO.COG MENZEL, UNSOELD 1936: AP.J. 84, 474 T(FE I, TI I EXCITATION) REMARKS : COMMENTS: OBSERVATIONS WERE DONE BETWEEN 1937-1945 CLASS : DTAA ------------------------------------------------------------------------ (423) LUCK, R.E., LAMBERT, D.L. 1981: ASTROPHYS.J. 245, 1018 ........................................................................ OBSERV. : PE, RETICON, 100A SECTIONS CENTERED AT 5380, 6300, 6385, 6425, 6560, 8710A, 0.2A, S/N=100 INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: DOAR, 150-250 ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: GIVE ABUNDANCES FOR C, N, O, FE CLASS : DTGMSA, R ======================================================================== HD 195633 BD +06 4557 G0VM (WEAK METALS) AR 20 29.9 DEC +06 21 MV = 8.56 FE/H = --- (L) ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, (L) ======================================================================== HD 196171 ALF IND K0III CN VAR... (EMISS H+K) AR 20 34.0 DEC -47 28 MV = 3.11 FE/H = 0 (I) ------------------------------------------------------------------------ ( 16) WARNER, B. 1965: MONTHLY NOTICES ROY.ASTRON.SOC. 129, 263 ........................................................................ OBSERV. : PG, RED RANGE, 13.6 A/MM INSTRUM.: RADCLIFFE 74-INCH, COUDE LINELIST: LW: WARNER 1964: COMM.UNIV.LONDON OBS. 65 ANALYSIS: COG, DIFF(SUN), THEOR.COG. FROM WRUBEL 1949: AP.J. 109, 66 T(COG SHIFTS), PE(IONIZATION) REMARKS : COMMENTS: CLASS : DTAA ======================================================================== HD 196662 TAU CAP B6III AR 20 36.5 DEC -15 08 MV = 5.22 FE/H = + (I) ------------------------------------------------------------------------ ( 94) ALLER, L.H., ROSS, J.E. 1967: THE MAGNETIC AND RELATED STARS, R.C.CAMERON ED., MONO BOOK CO., BALTIMORE, P.339 ........................................................................ OBSERV. : PG, 3200-4800A, 2 A/MM; 4800-6600A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: LTE(MIHALAS), EQU.WIDTHS VIA WEIGHTING FUNCTIONS, T(SCAN, COLOURS, IONIZATION), G(BALMER LINE PROFILES), F-VALUES: VARIOUS SOURCES REMARKS : COMMENTS: PRELIMINARY RESULTS CLASS : DTGMAA, (I) ======================================================================== HD 196378 PHI2 PAV F8V AR 20 35.9 DEC -60 43 MV = 5.12 FE/H = - (L) ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), (L) ======================================================================== HD 196725 TET DEL K3IAB: (EMISS H+K) AR 20 36.4 DEC +13 08 MV = 5.72 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 196755 KAP DEL G2IV (EMISS H+K) AR 20 36.7 DEC +09 55 MV = 5.05 FE/H = 0 L? ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (270) KUROCZKIN, D. WISZNIEWSKI, A. 1977: ACTA ASTON. 27, 145 ........................................................................ OBSERV. : GLEBOCKI, STROBEL 1970: ACTA ASTRON. 20, 361 INSTRUM.: LINELIST: 21 FE I LINES ANALYSIS: COG(WEIGHTING FUNCTIONS VIA LTE MODELS(PEYTREMANN 1974)) T(PREVIOUS WORK.....), G(EVOLUT.TRACKS), F-VALUES FROM MAY ET AL. 1974: A+A SUPPL. 18, 405 REMARKS : DERIVE FE ABUNDANCE ONLY COMMENTS: CLASS : TMA, L? ======================================================================== HD 197345 ALF CYG A2IAE AR 20 39.7 DEC +45 06 MV = 1.25 FE/H = ? I ------------------------------------------------------------------------ (189) GROTH, H.-G. 1961: Z.ASTROPHYS. 51, 206 AND 231 ........................................................................ OBSERV. : PG, 3075-8860A, 2.8+10+20+54 A/MM INSTRUM.: MT.WILSON 100-INCH (VIS, IR), MCDONALD (UV), HAMBURG OBS. LINELIST: LLWW, 800 ANALYSIS: LTE(UNBLANKETED), T+G(PROFILES OF HGAMMA..H10; BJ; WIDTHS OF HE I LINES, MG I/II IONIZATION; AL I/CA II RATIO), F-VALUES: VARIOUS SOURCES AS LISTED COMPARES OBS.AND CALC. PROFILES OF CA II K, MG II 4481, FE I 4045, SI II 3853, 3856, 4128 A REMARKS : DERIVES STELLAR F-VALUES COMMENTS: BEFORE THE REVISION OF FE F VALUES CLASS : TGMAA, I ------------------------------------------------------------------------ (114) PRZYBYLSKI, A. 1972: MONTHLY NOTICES ROY.ASTRON.SOC. 159, 155 ........................................................................ OBSERV. : DATA FROM (189) GROTH 1961: Z.ASTROPHYS. 51, 206 AND 231 INSTRUM.: LINELIST: ANALYSIS: COG, T(FE IONIZATION, OVERABUNDANCE OF ELEMENTS(??)), F-VALUES: FE I: GARZ, KOCK 1969, FE II: BASCHEK ET AL.1970 REMARKS : COMMENTS: CLASS : TA, I ======================================================================== HD 197989 EPS CYG K0III (EMISS H+K+MG(UV)) AR 20 44.2 DEC +33 47 MV = 2.50 FE/H = 0 R? ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 3954-4822A, 2 A/MM; 5325-6635A, 3 A/MM INSTRUM.: DAO 48-INCH, COUDE LINELIST: 800:, LLWW: KOELBLOED,VAN PARADIJS 1975: A+A SUPPL. 19, 101 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (254) PILACHOWSKI, C.A. 1977: ASTRON.ASTROPHYS. 54, 465 ........................................................................ OBSERV. : PG, ??? , 3.4-10 A/MM INSTRUM.: MAUNA KEA 2.2M, COUDE LINELIST: LW: TO BE PUBLISHED ??? ANALYSIS: LTE(CARBON, GINGERICH 1969), DIFF(EPS VIR), T(CONT.SLOPE 5400/6300A), G(MG II B LINE PROFILES, FE I/II, TI I/II, CR I/II IONIZATION), F-VALUES: VARIOUS SOURCES REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T+G(THEOR./EMPIR. COG) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 198149 ETA CEP K0IV (EMISS H+K) AR 20 44.3 DEC +61 39 MV = 3.41 FE/H = 0 R ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 3954-4822A, 2 A/MM; 5325-6635A, 3 A/MM INSTRUM.: DAO 48-INCH, COUDE LINELIST: 800:, LLWW: KOELBLOED,VAN PARADIJS 1975: A+A SUPPL. 19, 101 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T+G(THEOR./EMPIR. COG) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 198269 BD +17 4421 R (CH) AR 20 49.3 DEC +17 39 MV = 8.23 FE/H = --- (L) ------------------------------------------------------------------------ (108) LEE, P. 1974: ASTROPHYS.J. 192, 133 ........................................................................ OBSERV. : PG, 4380-6610A, 6.5-17.8 A/MM INSTRUM.: KPNO 0.4M, DAO 48-INCH LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(EPS VIR), T(V-R) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 200465 BD +38 4321A K3II-III AR 21 00.4 DEC +39 19 MV = 6.5 FE/H = 0 (I) ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA, (I) ======================================================================== HD 200905 XI CYG K4.5IB (EMISS H+K) AR 21 03.1 DEC +43 43 MV = 3.72 FE/H = 0 R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 5000-6650A, 6.5 A/MM INSTRUM.: MT.WILSON 100-INCH LINELIST: 800:, VAN PARADIJS 1973: A+A SUPPL. 11, 25 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: PROBABLY SUPERSEDED BY (388) CLASS : DTGMAA ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 201091 61 CYG A K5V (EMISS H+K, COMPOS.SPECTR.) AR 21 04.7 DEC +38 30 MV = 5.21 FE/H = 0 R ------------------------------------------------------------------------ (216) STROHBACH, P. 1970: ASTRON.ASTROPHYS. 6, 385 ........................................................................ OBSERV. : PG, 3800-4870A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LW, 160: ANALYSIS: MAKE A ROUGH COMPARISON WITH HD 156026, G(ABS.MAG.), T(SCAN 3800-12000A, LINES), REMARKS : SPECTRA ARE NOT SUITABLE FOR QUANTITATIVE ANALYSIS, THEREFORE NO DETAILS ABOUT THE MODEL ATMOSPHERE AND INDIVIDUAL ABUNDANCES ARE GIVEN COMMENTS: CLASS : (DTGMAA) ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : PG, ???? , 6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.PALOMAR 200-INCH LINELIST: 250 ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ------------------------------------------------------------------------ (255) HARTMANN, L., ANDERSON, C.M. 1977: ASTROPHYS.J. 215, 177 ........................................................................ OBSERV. : PG, 5900-6600A, 0.1 A INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: ANALYSIS: COG(SOLAR FE I COG(FOY 1972: A+A 18, 26), SHIFTS FROM LTE(CARBON, GINGERICH) MODELS), DIFF(SUN, HSRA), T(V-K, R-I), G(ASSUMED), T+G CHECKED WITH FE, TI, V, CA IONIZATION REMARKS : ALSO USE MODELS OF JOHNSON 1974: NCAR TECH.NOTE, STR-95 COMMENTS: CLASS : DTMAA, R ======================================================================== HD 201092 61 CYG B K7V AR 21 04.6 DEC +38 29 MV = 6.03 FE/H = 0 R ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 4.5+6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, R ------------------------------------------------------------------------ (255) HARTMANN, L., ANDERSON, C.M. 1977: ASTROPHYS.J. 215, 177 ........................................................................ OBSERV. : PG, 5900-6600A, 0.1 A INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: ANALYSIS: COG(SOLAR FE I COG(FOY 1972: A+A 18, 26), SHIFTS FROM LTE(CARBON, GINGERICH) MODELS), DIFF(SUN, HSRA), T(V-K, R-I), G(ASSUMED), T+G CHECKED WITH FE, TI, V, CA IONIZATION REMARKS : ALSO USE MODELS OF JOHNSON 1974: NCAR TECH.NOTE, STR-95 COMMENTS: CLASS : DTMAA, R ------------------------------------------------------------------------ (313) MOULD, J.R., 1978: ASTROPHYS.J. 226, 923 ........................................................................ OBSERV. : 1.5-2.5 MU, 1.5 A (= 4000-6600CM**-1, 0.3 CM**-1) INSTRUM.: KPNO 4M, FTS LINELIST: LW, 22 ANALYSIS: LTE(MOULD 1976), SPECTRUM SYNTHESIS, T(7540-10175 COLOUR), F-VALUES: DIFF(SUN), THEORETICAL VALUES REMARKS : COMMENTS: CLASS : (D)TMSA, L ======================================================================== HD 201626 BD +26 4091 G9P AR 21 07.8 DEC +26 25 MV = 8.13 FE/H = --- (I) ------------------------------------------------------------------------ ( 18) WALLERSTEIN, G., GREENSTEIN, J.L. 1964: ASTROPHYS.J. 139, 1163 ........................................................................ OBSERV. : PG, 4380-4600A, 9 A/MM, 5165-6800A, 6.7-13.5 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: ??? 262 ANALYSIS: COG, DIFF(EPS VIR), T(BVGRI) REMARKS : CH-STAR COMMENTS: BEFORE REVISION OF FE F-VALUES CLASS : DTAA, (I) ======================================================================== HD 201891 BD +17 4519 F8V-VI (SUBDWARF) AR 21 09.7 DEC +17 32 MV = 7.38 FE/H = --- (R) ------------------------------------------------------------------------ (298) CARNEY, B.W. 1979: ASTROPHYS.J. 233, 211 ........................................................................ OBSERV. : PG, 4070-4490A, 3.5 A/MM INSTRUM.: SAO 1.5M, ECHELLE, KRON EGC LINELIST: LW, 27 ANALYSIS: LTE(ATLAS), DIFF(SUN), T(R-I, V-K; SCAN: PASCHEN CONT), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 203608 GAM PAV F6V (SUBDWARF) AR 21 22.3 DEC -65 36 MV = 4.22 FE/H = -- R ------------------------------------------------------------------------ ( 45) DANZIGER, I.J. 1966: ASTROPHYS.J. 143, 527 ........................................................................ OBSERV. : PG, 4000-4900A, 6.7 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 142 ANALYSIS: COG(SOLAR COG FROM ALLER 1953: ASTROPHYSICS, RONALD PRESS), DIFF(SUN), T(UVBGRI, EXCITATION), PE(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 71) BUTCHER, H.R. 1972: ASTROPHYS.J. 176, 711 ........................................................................ OBSERV. : PG, 70A RANGE AT 4130A, 1 A/MM, 0.08A INSTRUM.: MT.STROMLO 1.9M, COUDE, ECHELLE, IT LINELIST: LW, 3 ANALYSIS: COG(15 FE I LINES, SOLAR COG, MILNE-EDDINGTON ATMOSPHERE), T(COG SHIFTS REL.TO MODELS OF CAYREL+JUGAKU 1963) REMARKS : PRESENTS PRELIMINARY RESULTS OF LARGER SURVEY CONSIDERS BA II 4130, EU II 4129, FE II 4128 ONLY COMMENTS: CLASS : DT(M)A ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3330-3900A, 4255-4350A, 7 A/MM INSTRUM.: RADCLIFFE 74-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, B-V, B-Y) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: SEE ALSO: CLEGG ET AL.1977: MNRAS 181, 31 CLASS : DTGMSA, R ------------------------------------------------------------------------ (419) STEENBOCK, W. 1983: ASTRON.ASTROPHYS. 126, 325 ........................................................................ OBSERV. : PG, 3500-6050A, 3.3 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LW, 25: ANALYSIS: LTE(SCALED SOLAR T-TAU RELATION, ATLAS), DIFF(SUN), T(VRI, MG I B LINE WINGS), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVE BA, FE, MG ABUNDANCES FROM SELECTED ISOLATED LINES COMMENTS: CLASS : DTGMA, R ======================================================================== HD 204543 BD -04 5460 G0 (WEAK METALS) AR 21 26.9 DEC -03 44 MV = 8.6 FE/H = --- (R) ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 204613 BD +56 2578 K0 (SUBGIANT CH, WEAK METALS) AR 21 26.2 DEC +57 06 MV = 8.31 FE/H = - R ------------------------------------------------------------------------ (A30) LUCK, R.E., BOND, H.E. 1982: ASTROPHYS.J. 259, 792 ........................................................................ OBSERV. : PG, 3800-5000A, 9 A/MM; 50A SECTIONS IN 5100-7800A, 0.2A, S/N= 30..50 (RETICON) INSTRUM.: MT.WILSON 100-INCH, COUDE, RETICON, MT.PALOMAR 200-INCH LINELIST: 200 OR MORE ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A29) SNEDEN, C. 1983: PUBL.ASTRON.SOC.PACIFIC 95, 745 ........................................................................ OBSERV. : PE, 50A SECTIONS AT 4230, 4370, 4730 A, 0.3 A, S/N= 100 (D) 95A SECTIONS AT 6325 A, 0.3 A, S/N= 75..200 (RETICON) INSTRUM.: MCDONALD 2.7M, COUDE, DIGICON, RETICON LINELIST: 20: ATOMIC LINES; C2, OI, CH FEATURES ANALYSIS: LTE(ATLAS), SPECTRUM SYNTHESIS FOR MOLECULAR FEATURES, T+G(FROM (A30) LUCK BOND 1982: AP.J. 259, 792: T(B-Y, FE I EXCITATION), G(FE I/II IONIZATION)), F-VALUES: DIFF(SUN, HOLWEGER MUELLER MODEL) REMARKS : FINDS LOWER MICROTURBULENCE THAN IN (A30) COMMENTS: CLASS : D(TG)MSA, R ======================================================================== HD 204867 BET AQR G0IB (EMISS H+K+MG(UV)) AR 21 28.9 DEC -05 47 MV = 2.91 FE/H = 0 R ------------------------------------------------------------------------ (277) LUCK, R.E. 1977: ASTROPHYS.J. 218, 752 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MC.DONALD 2.1M, COUDE LINELIST: ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR. COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: PROBABLY SUPERSEDED BY (388) CLASS : DTGMAA ------------------------------------------------------------------------ (352) FOY, R. 1981: ASTRON.ASTROPHYS. 103, 135 ........................................................................ OBSERV. : DATA FROM LUCK 1977: AP.J. 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T(LUCK), G(IONIZATION FE, TI, CR), F-VALUES: FOY 1972: A+A 18, 26 REMARKS : REANALYIS, GIVE RESULTS ON FE/H ONLY COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (423) LUCK, R.E., LAMBERT, D.L. 1981: ASTROPHYS.J. 245, 1018 ........................................................................ OBSERV. : PE, RETICON, 100A SECTIONS CENTERED AT 5380, 6300, 6385, 6425, 6560, 8710A, 0.2A, S/N=100 INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: DOAR, 150-250 ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : T+G FROM LUCK 1977: ASTROPHYS.J. 212, 743 COMMENTS: GIVE ABUNDANCES FOR C, N CLASS : DMSA ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 218, 752 INSTRUM.: SEE ALSO: AP.J. 212, 797 LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 205512 72 CYG K1III (EMISS H+K, CN) AR 21 32.7 DEC +38 19 MV = 4.90 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 206859 9 PEG G5IB (EMISS H+K) AR 21 42.1 DEC +17 07 MV = 4.34 FE/H = 0 R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 5000-6650A, 6.5 A/MM INSTRUM.: MT.WILSON 100-INCH LINELIST: 800:, VAN PARADIJS 1973: A+A SUPPL. 11, 25 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: PROBABLY SUPERSEDED BY (388) CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 206952 11 CEP K1III (EMISS H+K) AR 21 41.2 DEC +71 05 MV = 4.56 FE/H = 0 (L) ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, (L) ======================================================================== HD 207089 12 PEG K0IAB: (EMISS H+K) AR 21 43.8 DEC +22 43 MV = 5.29 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 207489 BD +38 4611 F5IB AR 21 46.2 DEC +38 43 MV = 7.16 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 207673 HR 8345 A2IB AR 21 47.6 DEC +40 55 MV = 6.48 FE/H = ? (L) ------------------------------------------------------------------------ (172) AYDIN, C. 1972: ASTRON.ASTROPHYS. 19, 369 ........................................................................ OBSERV. : PG, 3710-4860A, 12.4 A/MM INSTRUM.: OHP 1.5M, 1.9M, COUDE LINELIST: 280:, AYDIN 1972: ASTRON.ASTROPHYS.SUPPL. 7, 331 ANALYSIS: COG, DIFF(ALF CYG), T+G(HBETA, HGAMMA, BALMER DISC.), PE(FE I/II IONIZATION, INGLIS-TELLER) F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVES FE, TI, CR ABUNDANCES ONLY COMMENTS: CLASS : DTGA, (L) ======================================================================== HD 207978 15 PEG F6IV-V WVAR AR 21 50.3 DEC +28 34 MV = 5.50 FE/H = -- R ------------------------------------------------------------------------ (317) GEHREN, T. 1979: ASTRON.ASTROPHYS. 75, 73 ........................................................................ OBSERV. : PG, 4400-6820A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 480:, LLWW: GEHREN ET AL.1978: A+A SUPPL. 31, 297 ANALYSIS: LTE(T-TAU SCALED FROM EMPIRICAL SOLAR MODEL: HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), T(LINE PROFILES OF HALFA, HGAMMA, HDELTA), G(IONIZATION SI, TI, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : DATA FROM (317) GEHREN 1979: A+A 75, 73 INSTRUM.: LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HGAMMA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), L ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 208606 HR 8374 G8IAB: (EMISS H+K) AR 21 53.8 DEC +61 18 MV = 6.13 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 208776 BD +03 4644 G0V AR 21 56.0 DEC +03 32 MV = 6.94 FE/H = 0 (R) ------------------------------------------------------------------------ ( 90) ZIELKE, G. 1970: ASTRON.ASTROPHYS. 6, 206 ........................................................................ OBSERV. : PG, 3900-4800A, 10 A/MM; 4800-6700A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LESS THAN 600:, LLWW: ZIELKE 1970: A+A SUPPL. 2, 205 ANALYSIS: LTE(T-TAU SCALED FROM SUN: HOLWEGER 1967: Z.AP. 65, 365), DIFF(HD 136202), T(PROFILES OF HALFA, HBETA, HGAMMA, HDELTA; BVGRI; LINE EXCITATION), G(IONIZATION SI, SC, TI, V, CR, FE, SR), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 208906 BD +29 4550 F8V-VI (SUBDWARF) AR 21 56.5 DEC +29 35 MV = 6.94 FE/H = -- R ------------------------------------------------------------------------ ( 90) ZIELKE, G. 1970: ASTRON.ASTROPHYS. 6, 206 ........................................................................ OBSERV. : PG, 3900-4800A, 10 A/MM; 4800-6700A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LESS THAN 600:, LLWW: ZIELKE 1970: A+A SUPPL. 2, 205 ANALYSIS: LTE(T-TAU SCALED FROM SUN: HOLWEGER 1967: Z.AP. 65, 365), DIFF(HD 136202), T(PROFILES OF HALFA, HBETA, HGAMMA, HDELTA; BVGRI; LINE EXCITATION), G(IONIZATION SI, SC, TI, V, CR, FE, SR), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3800-4700A, 13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ======================================================================== HD 209100 EPS IND K4.5V (EMISS H+K) AR 21 59.5 DEC -57 00 MV = 4.69 FE/H = 0 (R) ------------------------------------------------------------------------ (320) KOLLATSCHNY, W. 1980: ASTRON.ASTROPHYS. 86, 308 ........................................................................ OBSERV. : PG, 3950-5000A, 3.3 A/MM; 5500-6700A, 5.1 A/MM INSTRUM.: ESO 1.5M LINELIST: LW, 220:, 800 LINES IDENTIFIED AND MEASURED ANALYSIS: LTE, T(BVRI), G(ABS.MAG.), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 209459 21 PEG B9.5V AR 22 00.9 DEC +11 09 MV = 5.80 FE/H = - (R) ------------------------------------------------------------------------ (394) SADAKANE, K. 1981: PUBL.ASTRON.SOC.PACIFIC 93, 587 ........................................................................ OBSERV. : PG, 3850-4640A, 2.3 A/MM (DAO); HGAMMA, HDELTA, 10 A/MM (OK) INSTRUM.: DAO; OKAYAMA OBS. LINELIST: LLWW, 150: ANALYSIS: LTE(ATLAS), T+G(B-V, B-Y, M1, C1, BETA; HGAMMA, HDELTA PROFILES; FE I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED COMPARE OBS.AND CALC. SCAN 3300..7000 A REMARKS : COMMENTS: CLASS : TGMAA, (R) ======================================================================== HD 209750 ALF AQR G2IB (EMISS H+K) AR 22 03.2 DEC -00 34 MV = 2.90 FE/H = 0 R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 5000-6650A, 6.5 A/MM INSTRUM.: MT.WILSON 100-INCH LINELIST: 800:, VAN PARADIJS 1973: A+A SUPPL. 11, 25 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (277) LUCK, R.E. 1977: ASTROPHYS.J. 218, 752 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MC.DONALD 2.1M, COUDE LINELIST: ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR. COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: PROBABLY SUPERSEDED BY (388) CLASS : DTGMAA ------------------------------------------------------------------------ (352) FOY, R. 1981: ASTRON.ASTROPHYS. 103, 135 ........................................................................ OBSERV. : DATA FROM LUCK 1977: AP.J. 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T(LUCK), G(IONIZATION FE, TI, CR), F-VALUES: FOY 1972: A+A 18, 26 REMARKS : REANALYIS, GIVE RESULTS ON FE/H ONLY COMMENTS: CLASS : DGMA, R ------------------------------------------------------------------------ (423) LUCK, R.E., LAMBERT, D.L. 1981: ASTROPHYS.J. 245, 1018 ........................................................................ OBSERV. : PE, RETICON, 100A SECTIONS CENTERED AT 5380, 6300, 6385, 6425, 6560, 8710A, 0.2A, S/N=100 INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: DOAR, 150-250 ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : T+G FROM LUCK 1977: ASTROPHYS.J. 212, 743 COMMENTS: GIVE ABUNDANCES FOR C, N CLASS : DMSA ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 218, 752 INSTRUM.: SEE ALSO: AP.J. 212, 797 LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 209975 19 CEP O9IB AR 22 03.6 DEC +62 02 MV = 5.11 FE/H = 0 (L) ------------------------------------------------------------------------ (376) TAKADA, M. 1977: PUB.ASTRON.SOC.JAPAN 29, 439 ........................................................................ OBSERV. : PG, 3510-6660A, 4+10+20 A/MM INSTRUM.: OKAYAMA OBS. 1.9M, COUDE LINELIST: LLWW, 100: ANALYSIS: LTE(ATLAS), T+G(WIDTHS OF HGAMMA, HDELTA, HEPSILON; BALMER JUMP; N II/III, SI III/IV IONIZATION; U B C0), F-VALUES: VARIOUS SOURCES (1964-1971) AS LISTED, CHECKS: SCAN 3200-8060A, PROFILES OF HGAMMA, HDELTA, HEPSILON, HE I 4471, 4026, 3820, 4388, 4144, 4009 A HE II 4686, 5412, 4542 A REMARKS : OBSERVATIONAL DATA IS ALSO COMPARED RESULTS FROM NLTE/L MODELS (MIHALAS 1972-1975) COMMENTS: CLASS : TGM(N)AA, (L) ======================================================================== HD 210221 HR 8443 A3IB AR 22 05.6 DEC +53 04 MV = 6.14 FE/H = ? (L) ------------------------------------------------------------------------ (172) AYDIN, C. 1972: ASTRON.ASTROPHYS. 19, 369 ........................................................................ OBSERV. : PG, 3710-4860A, 12.4 A/MM INSTRUM.: OHP 1.5M, 1.9M, COUDE LINELIST: 280:, AYDIN 1972: ASTRON.ASTROPHYS.SUPPL. 7, 331 ANALYSIS: COG, DIFF(ALF CYG), T+G(HBETA, HGAMMA, BALMER DISC.), PE(FE I/II IONIZATION, INGLIS-TELLER) F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVES FE, TI, CR ABUNDANCES ONLY COMMENTS: CLASS : DTGA, (L) ======================================================================== HD 210295 BD -14 6222 G5 (WEAK METALS) AR 22 07.0 DEC -13 51 MV = 9.57 FE/H = --- R? ------------------------------------------------------------------------ (346) PETERSON, R.C. 1981: ASTROPHYS.J.SUPPL. 45, 421 ........................................................................ OBSERV. : PG, IT, 5540-6750A, 3.1 A/MM INSTRUM.: KPNO 4M, ECHELLE, CARNEGIE IT LINELIST: LLWW, 300: ANALYSIS: LTE(ATLAS, GUSTAFSSON), T(FE I EXCITATION), G(FE II/I IONIZATION), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: CLASS : (D)TGMA, R? ------------------------------------------------------------------------ (344) PETERSON, R.C. 1981: ASTROPHYS.J. 244, 989 ........................................................................ OBSERV. : DATA FROM (346) PETERSON 1980: ASTROPHYS.J.SUPPL. 45, 421 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON, ATLAS), T(R-I), G(ASSUMED), F-VALUES DIFF(SUN) REMARKS : DERIVES NA ... CU ABUNDANCE RATIOS RELATIVE TO FE COMMENTS: CLASS : DTMA ======================================================================== HD 210334 1 AR LAC A G2IV+... (EMISS H+K) AR 22 06.7 DEC +45 30 MV = -.-- FE/H = - (I?) ------------------------------------------------------------------------ (272) NAFTILAN, S.A., DRAKE, S.A. 1977: ASTROPHYS.J. 216, 508 ........................................................................ OBSERV. : PG, CENTERED AT 4050A, 11 A/MM; AT 5400+6560A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: COG(WRUBEL 1950, FE I), T+G(BINARY MASS+LUMINOSITY; HGAMMA; COG; PHOTOMETRY) REMARKS : CONTAMINATION OF SPECTRUM BY SECONDARY STAR DID NOT PERMIT A MORE TAHN A CRUDE ANALYSIS COMMENTS: DESCRIPTION OF ANALYSIS IS NOT VERY DETAILLED CLASS : TGAA, (I?) ======================================================================== HD 210334 2 AR LAC B K0III (EMISS H+K) AR 22 06.7 DEC +45 30 MV = -.-- FE/H = -- (L?) ------------------------------------------------------------------------ (272) NAFTILAN, S.A., DRAKE, S.A. 1977: ASTROPHYS.J. 216, 508 ........................................................................ OBSERV. : PG, CENTERED AT 4050A, 11 A/MM; AT 5400+6560A, 16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: ANALYSIS: LTE(CARBON, GINGERICH 1969 ?), SPECTRUM SYNTHESIS, T+G(BINARY MASS+LUMINOSITY; HGAMMA; COG; PHOTOMETRY) REMARKS : COMMENTS: DESCRIPTION OF ANALYSIS IS NOT VERY DETAILLED CLASS : TGMSAA, (L?) ======================================================================== HD 210745 ZET CEP K1.5IB (EMISS H+K+MG(UV)) AR 22 09.1 DEC +57 57 MV = 3.35 FE/H = 0 R ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: PROBABLY SUPERSEDED BY (388) CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 211391 TET AQR G8III (EMISS H+K) AR 22 14.2 DEC -08 02 MV = 4.16 FE/H = 0 (L) ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, (L) ======================================================================== HD 211998 NU IND A3V+... AR 22 20.4 DEC -72 30 MV = 5.29 FE/H = --- R ------------------------------------------------------------------------ ( 71) BUTCHER, H.R. 1972: ASTROPHYS.J. 176, 711 ........................................................................ OBSERV. : PG, 70A RANGE AT 4130A, 1 A/MM, 0.08A INSTRUM.: MT.STROMLO 1.9M, COUDE, ECHELLE, IT LINELIST: LW, 3 ANALYSIS: COG(15 FE I LINES, SOLAR COG, MILNE-EDDINGTON ATMOSPHERE), T(COG SHIFTS REL.TO MODELS OF CAYREL+JUGAKU 1963) REMARKS : PRESENTS PRELIMINARY RESULTS OF LARGER SURVEY CONSIDERS BA II 4130, EU II 4129, FE II 4128 ONLY COMMENTS: CLASS : DT(M)A ------------------------------------------------------------------------ (208) HEARNSHAW, J.B. 1975: ASTRON.ASTROPHYS. 38, 271 ........................................................................ OBSERV. : PG, 4150-4800A, 6.7+10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(HALFA, R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUNDANCES ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (419) STEENBOCK, W. 1983: ASTRON.ASTROPHYS. 126, 325 ........................................................................ OBSERV. : PG, 4650-6050A, 3.3 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: LW, 25: ANALYSIS: LTE(SCALED SOLAR T-TAU RELATION, ATLAS), DIFF(SUN), T(R-I, MG I B LINE WINGS), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN) REMARKS : DERIVE BA, FE, MG ABUNDANCES FROM SELECTED ISOLATED LINES COMMENTS: CLASS : DTGMA, R ======================================================================== HD 212330 HR 8531 G3IV AR 22 21.6 DEC -58 03 MV = 5.31 FE/H = 0 (L) ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), (L) ======================================================================== HD 213009 DEL1 GRU G7III AR 22 26.3 DEC -43 45 MV = 3.97 FE/H = 0 (R) ------------------------------------------------------------------------ (325) FOY, R. 1981: ASTRON.ASTROPHYS. 93, 315 ........................................................................ OBSERV. : PG, ??? 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FE I/II IONIZATION, R-I, WEAK AND STRONG MG I LINES, WEAK AND STRONG FE I LINES) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 213320 SIG AQR A0IVS AR 22 28.0 DEC -10 56 MV = 4.82 FE/H = + (R) ------------------------------------------------------------------------ (354) ADELMAN, S.J., NASSON, M.A. 1980: PUBL.ASTRON.SOC.PACIFIC 92, 346 ........................................................................ OBSERV. : PG, 3300-7100A, 4.3+8.9 A/MM INSTRUM.: MT.WILSON 100-INCH, KPNO 4M, COUDE LINELIST: LLWW, 200: ANALYSIS: LTE(ATLAS), T+G(SCAN 3300-7100A, HGAMMA PROFILE), F-VALUES: VARIOUS SOURCES AS LISTED, REMARKS : COMPARE ABUNDANCES WITH SOLAR ONES THAT HAD BEEN DERIVED WITH THE SAME F-VALUES COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 214080 BD -17 6554 B1IB AR 22 33.6 DEC -16 39 MV = 6.83 FE/H = 0 (L) ------------------------------------------------------------------------ (A26) KEENAN, F.P., LENNON, D.J. 1984: ASTRON.ASTROPHYS. 130, 179 ........................................................................ OBSERV. : PG, 3450-4800A, 6.8 A/MM INSTRUM.: SAAO 1.9M, COUDE LINELIST: LW, 60: ANALYSIS: LTE(KLINGLESMITH), T(C1, LTE(MORTON)), G(HGAMMA PROFILE, HEPSILON WIDTH), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : TGMAA, L ======================================================================== HD 214539 SAO 255281 B8/B9IB (BLUE STRAGGLER) AR 22 37.3 DEC -67 57 MV = 7.27 FE/H = --- (L) ------------------------------------------------------------------------ (115) PRZYBYLSKI, A. 1969: MONTHLY NOTICES ROY.ASTRON.SOC. 146, 71 ........................................................................ OBSERV. : PG, 3670-6563A, 10.2+20.4 A/MM INSTRUM.: MT.STROMLO, COUDE LINELIST: LLWW, 200:, USED FOR ANALYSIS: 113 ANALYSIS: COG, DIFF(ETA LEO, 13 MON), THEOR.COG FROM WRUBEL 1949, T+PE(FE IONIZATION) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 214994 OMI PEG A1IV AR 22 39.4 DEC +29 03 MV = 4.79 FE/H = 0 R ------------------------------------------------------------------------ (145) CONTI, P.S., STROM, S.E. 1968: ASTROPHYS.J. 154, 975 ........................................................................ OBSERV. : PG, 3300-6250A, 4.5+6.7 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 300: ANALYSIS: LTE(STROM), T+G(FE I EXCITATION, FEI/II IONIZATION) REMARKS : COMMENTS: BVI COLOURS ARE NOT EXPLICITLY COMPARED WITH MODEL COLOURS CLASS : TGMAA, L ------------------------------------------------------------------------ (374) WOLFF, S.C. 1970: ASTROPHYS.J.SUPPL. 15, 21 ........................................................................ OBSERV. : PG, 3860-4620A, 8 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LW, 22 SELECTED UNBLENDED LINES ANALYSIS: COG(WRUBEL 1949), T(SCAN 4000-8800A, LTE(MIHALAS 1966)), G(HGAMMA PROFILES, LTE(MIHALAS 1966)), F-VALUES: WARNER 1967, CORLISS, BOZMAN 1962 REMARKS : USES ONLY ONE OR TWO LINES PER ION, MOST OF WHICH LIE ON THE COG'S FLAT PORTION. COMMENTS: THIS STAR SERVES AS STANDARD FOR STUDY OF AP STARS CLASS : TG(M)A ------------------------------------------------------------------------ (142) ADELMAN, S.J. 1973: ASTROPHYS.J. 183, 95 ........................................................................ OBSERV. : PG, 3850-3870A, 3968-4650A, 4.5 A/MM INSTRUM.: LICK, MT.PALOMAR 200-INCH, COUDE LINELIST: ANALYSIS: COG(LTE(ATLAS)), T(SCAN), G(HGAMMA PROFILE) REMARKS : COMMENTS: CLASS : TGMAA, L ------------------------------------------------------------------------ (265) ALLEN, M.S. 1977: ASTROPHYS.J. 213, 121 ........................................................................ OBSERV. : PG, 3700-4150A, 4200-4650A, 2.4 A/MM, 0.074A (FWHM) INSTRUM.: DAO 1.2M, COUDE, IMAGE SLICER LINELIST: 75, DAOR ANALYSIS: LTE(KCP 1969), T+G(UBV, HGAMMA, FE I/II IONIZATION) F-VALUES: EXPERIMENTAL, THEORETICAL, SOLAR REMARKS : DERIVES ABUNDANCES FOR FE, SR, Y, ZR ONLY COMMENTS: USES STAR AS COMPARISON FOR HG-MN STARS CLASS : (D)TGMA, L ------------------------------------------------------------------------ (256) MITTON, J. 1977: ASTRON.ASTROPHYS.SUPPL. 27, 35 ........................................................................ OBSERV. : PG, 3470-4680A, 4.5 A/MM (MT.W.), 10 A/MM (RGO) INSTRUM.: MT.WILSON 100-INCH; RGO 0.76M LINELIST: LLWW, 300: ANALYSIS: COG, DIFF(ALF CMI), T(FE I EXCITATION), TEFF+G(HGAMMA PROFILES, LTE(GINGERICH 1969), GRIEM THEORY), F-VALUES: CORLISS, WARNER 1963 REMARKS : EQU.WIDTHS FROM DIFFERENT SPECTRA WERE DIFFERENT BY 15 % COMMENTS: CLASS : DTG(M)AA, R ======================================================================== HD 215104 RHO GRU K0III AR 22 40.6 DEC -41 40 MV = 4.85 FE/H = 0 (R) ------------------------------------------------------------------------ (325) FOY, R. 1981: ASTRON.ASTROPHYS. 93, 315 ........................................................................ OBSERV. : PG, ??? 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FE I/II IONIZATION, R-I, WEAK AND STRONG MG I LINES, WEAK AND STRONG FE I LINES) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 216143 BD -07 5873 G5 (WEAK METALS) AR 22 47.9 DEC -07 11 MV = 8.2 FE/H = ---- (R) ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 216228 IOT CEP K0III (EMISS H+K+MG(UV)) AR 22 47.9 DEC +65 56 MV = 3.52 FE/H = 0 R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 3954-4822A, 2 A/MM; 5325-6635A, 3 A/MM INSTRUM.: DAO 48-INCH, COUDE LINELIST: 800:, LLWW: KOELBLOED,VAN PARADIJS 1975: A+A SUPPL. 19, 101 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 216385 SIG PEG F7IV AR 22 49.9 DEC +09 34 MV = 5.64 FE/H = - R ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 216437 RHO IND G2.5IV AR 22 51.2 DEC -70 20 MV = 6.05 FE/H = 0 (L) ------------------------------------------------------------------------ (326) GEHREN, T. 1981: ASTRON.ASTROPHYS. 100, 97 ........................................................................ OBSERV. : PG, HALFA, HBETA, 3.3+12.5 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(SCALED FROM HOLWEGER'S EMPIRICAL SOLAR MODEL), T(HALFA, HBETA PROFILES), G(???), SPECTRUM SYNTHESIS REMARKS : DERIVES TEMPERATURE CALIBRATION OF B-Y, B-V, R-I INDICES FOR TEFF = 5600..6400 K COMMENTS: GRAVITY AND METAL ABUNDANCES ESTIMATED ONLY CLASS : DTS(A), (L) ======================================================================== HD 216735 RHO PEG A1V AR 22 52.7 DEC +08 33 MV = 4.90 FE/H = ? (L) ------------------------------------------------------------------------ (174) BASCHEK, B., SEARLE, L. 1969: ASTROPHYS.J. 155, 537 ........................................................................ OBSERV. : PG, 3933-6370A, 4.5-15 A/MM; PG, IT, 7700-8600A, 20 OR 40 A/MM INSTRUM.: MT.WILSON 100-INCH, MT.STROMLO 74-INCH, COUDE LINELIST: LW, 45: ANALYSIS: COG(HUNGER 1955, WRUBEL 1949), DIFF(ALF LYR), T(SCAN 3390..10870A), G(HGAMMA, LTE(MIHALAS 1966)), PE(FE I/II) REMARKS : COMMENTS: CLASS : DTG(M)AA, (L) ======================================================================== HD 216763 DEL PSA G8III AR 22 53.2 DEC -32 48 MV = 4.21 FE/H = 0 (R) ------------------------------------------------------------------------ (325) FOY, R. 1981: ASTRON.ASTROPHYS. 93, 315 ........................................................................ OBSERV. : PG, ??? 12.4 A/MM INSTRUM.: ESO 1.5M, COUDE LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FE I/II IONIZATION, R-I, WEAK AND STRONG MG I LINES, WEAK AND STRONG FE I LINES) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 216946 HR 8726 K5IAB: (EMISS H+K) AR 22 54.2 DEC +49 28 MV = 4.95 FE/H = 0 R ------------------------------------------------------------------------ (277) LUCK, R.E. 1977: ASTROPHYS.J. 218, 752 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MC.DONALD 2.1M, COUDE LINELIST: ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR. COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 218, 752 INSTRUM.: SEE ALSO: AP.J. 212, 797 LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 217014 51 PEG G2.5IVA AR 22 55.0 DEC +20 30 MV = 5.49 FE/H = 0 (L) ------------------------------------------------------------------------ ( 86) HEARNSHAW, J.B. 1972: MEM.ROY.ASTRON.SOC. 77, 55 ........................................................................ OBSERV. : PG, 4460-4920A, 5500-6800A, 6.7-10.2 A/MM INSTRUM.: MT.STROMLO 1.9M, COUDE LINELIST: LLWW, 376 ANALYSIS: COG, DIFF(SUN), T(SCAN 4036-7530A, R-I, HALFA) REMARKS : DERIVES ALSO GRAVITY FROM METALLICITY AND ELECTRON PRESSURE COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 217476 HR 8752 G0IAB: (EMISS H+K) AR 22 59.0 DEC +56 41 MV = 5.00 FE/H = 0 R ------------------------------------------------------------------------ (240) FRY, M.A., ALLER, L.H. 1975: ASTROPHYS.J.SUPPL. 29, 55 ........................................................................ OBSERV. : PG, 3960-6610A, 4-16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 560: ANALYSIS: LTE(CARBON, GINGERICH 1969 ?), SPECTRUM SYNTHESIS, T(FE I, CR I, TI I EXCITATION), G(FE I/II, CR I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : DTGMSAA, R ------------------------------------------------------------------------ (236) LUCK, R.E. 1975: ASTROPHYS.J. 202, 743 ........................................................................ OBSERV. : PG, 3430-6780A, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2M LINELIST: LLWW, 260: ANALYSIS: COG(FROM LTE(JOHNSON 1974: NCAR TECH.NOTE 95; ATLAS) MODELS) DIFF(SUN(HSRA), EPS VIR(LTE(ATLAS))), T(FE I EXCITATION), G(FE I/II IONIZATION, ABS.MAG.+EVOL.TRACKS) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 217906 BET PEG M2.5II-III (EMISS MG(UV)) AR 23 01.3 DEC +27 49 MV = 2.42 FE/H = - R ------------------------------------------------------------------------ (247) HANNI, L., KIPPER, M. 1975: PUBL.TARTU ASTROFIZ. OBS. 43, 51 ........................................................................ OBSERV. : PG, 5050-6150A, 4 A/MM INSTRUM.: 100-INCH LINELIST: LLWW, 600: ANALYSIS: COG, T(???), F-VALUES WOLNIK ET AL.1970: AP.J. 162, 1037 (?) COMPARISON WITH THEOR. COG OF WRUBEL 1949: AP.J. 109, 66 REMARKS : COMMENTS: I CAN'T READ RUSSIAN WELL CLASS : TAA ------------------------------------------------------------------------ (A10) SMITH, V.V., LAMBERT, D.L. 1985: ASTROPHYS.J. 294, 326 ........................................................................ OBSERV. : PE, REGIONS BETWEEN 7330-7600 A, 0.2 A (RETICON) 1.6 + 2.2 MICRON (4500 CM**-1), 0.05 CM**-1 (FTS) INSTRUM.: MCDONALD 2.7M, COUDE, RETICON; KPNO 4M, FTS LINELIST: LW, 29 ATOMIC + 60 MOLECULAR LINES ANALYSIS: LTE(JOHNSON), DIFF(ALF TAU), T(V-K), G(ABS.MAG.+EVOL.TRACKS) F-VALUES: CF. LAMBERT ET AL. 1984: AP.J. 284, 223 REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 218470 5 AND F5V AR 23 05.5 DEC +49 01 MV = 5.70 FE/H = - (R) ------------------------------------------------------------------------ ( 91) FALIPOU, M.A. 1973: ASTRON.ASTROPHYS. 22, 445 ........................................................................ OBSERV. : PG, ??? , 9.7+12.4 A/MM INSTRUM.: OHP 1.5M, 1.9M, COUDE LINELIST: DAOR, 550: ANALYSIS: LTE(HOMOLOGOUS TO CARBON, GINGERICH 1969), DIFF(SUN, HSRA), T+G(HBETA PROFILE, FE I/II, TI I/II, CR I/II IONIZATION), ANALYZE NA I D, MG I B LINE PROFILES REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 218396 HR 8799 A5V AR 23 05.0 DEC +20 52 MV = 5.99 FE/H = --- (R) ------------------------------------------------------------------------ (A04) GEHREN, T. 1977: ASTRON.ASTROPHYS. 59, 315 ........................................................................ OBSERV. : PG, 3700-6000A, 4.5-15 A/MM INSTRUM.: MT.WILSON 100-INCH, ESO 1.5M, COUDE LINELIST: LLWW, 260, COMPLETE LIST OF 1500 LINES: DAOR ANALYSIS: LTE(UNBLANKETED), T+G(PROFILES OF HALFA, HGAMMA, HDELTA; MG, FE IONIZATION; UBV, UBY, C1; INGLIS-TELLER ON BALMER(20,21)), F-VALUES: DIFF(SUN) VIA EMPIRICAL SOLAR MODEL OF HOLWEGER, MUELLER 1974: SOLAR PHYS. 39, 19), REMARKS : COMMENTS: CLASS : (D)TGMAA, (R) ======================================================================== HD 218502 BD -15 6355 F5 (WEAK METALS) AR 23 06.0 DEC -15 19 MV = 8.5 FE/H = --- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-5200A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 218658 PI CEP G2III (EMISS H+K) AR 23 06.3 DEC +75 07 MV = 4.41 FE/H = 0 (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 218857 BD -17 6692 G0 (WEAK METALS) AR 23 08.8 DEC -16 31 MV = 8.72 FE/H = ---- (R) ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : PG, 3800-5000A, 10 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, LESS THAN 340 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FE I LINES), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN), HOLWEGER MODEL REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 219134 HR 8832 K3V (EMISS H+K) AR 23 10.9 DEC +56 54 MV = 5.56 FE/H = 0 R ------------------------------------------------------------------------ ( 41) CAYREL DE STROBEL, G. 1966: ANN.ASTROPHYS. 29, 413 ........................................................................ OBSERV. : PG, 4400-6800A, 9.7+12.4 A/MM, 0.3A INSTRUM.: OHP 1.9M, COUDE LINELIST: LLWW, 260: ANALYSIS: COG, DIFF(SUN), THEOR.COG FROM LTE MODELS BY CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495; T+G(TI, FE, CR IONIZATION, UVBGRI, LINE PROFILES OF MG I B, NA I D, HALFA) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (224) CAYREL DE STROBEL, G., CHAUVE-GODARD, J., HERNANDEZ, G., VAZIAGA, M. J. 1970: ASTRON.ASTROPHYS. 7, 408 ........................................................................ OBSERV. : DATA FROM ( 41) CAYREL DE STROBEL 1966: ANN.ASTR. 29, 413 INSTRUM.: LINELIST: LW, 12 ANALYSIS: LTE(CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495), DIFF(SUN) T(IONIZ.TEMP. FROM PREVIOUS ANALYSES) REMARKS : RE-ANALYZE OBSERVATIONAL MATERIAL TAKEN BY REF.(41) DERIVE FE, NA ABUND. COMMENTS: CLASS : D(T)MA, L ------------------------------------------------------------------------ (216) STROHBACH, P. 1970: ASTRON.ASTROPHYS. 6, 385 ........................................................................ OBSERV. : DATA FROM ( 41) CAYREL DE STROBEL 1966: ANN.ASTR. 29, 413 INSTRUM.: LINELIST: ANALYSIS: LTE(UNBLANKETED), DIFF(SUN), T(B-V, VRI, G-I; WINGS OF HALFA, HBETA; EXCITATION+IONIZATION FE, CR, TI, SC; WIDTHS OF RESONANCE LINES OF NA I, CA I, CR I, AND FE I (MULTIPL. 41..43); STRENGTH OF MGH BAND), G(ABS.MAG.+PARALLAX), REMARKS : COMMENTS: CLASS : DT(G)MAA, L ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7+9.0 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (150) PERRIN, M.-N., CAYREL, R., CAYREL DE STROBEL, G. 1975: ASTRON.ASTROPHYS. 39, 97 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 AND FROM ( 41) CAYREL 1966: ANN.ASTROPHYS. 29, 413 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), THEOR. COG FROM LTE MODELS(PEYTREMANN 1970), T+G(R-I, V-K, G-I; IONIZATION FE, TI, CR; EXCITATION) F-VALUES: FOY 1972: A+A 18, 26 REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (275) OINAS, V. 1977: ASTRON.ASTROPHYS. 61, 17 ........................................................................ OBSERV. : DATA FROM (151) OINAS 1974: AP.J.SUPPL. 27, 391 INSTRUM.: LINELIST: ANALYSIS: LTE(CARBON, GINGERICH; ATLAS), DIFF(SUN), T(SCAN ???), G(ASSUMED) F-VALUES: MAY 1974: A+A SUPPL. 18, 405 (FE I) REMARKS : ALSO DERIVES GRAVITIES FROM NEUTRAL/IONIC LINES COMMENTS: CLASS : DTMAA, L ======================================================================== HD 219615 GAM PSC K0III: (EMISS H+K+MG(UV)) AR 23 14.6 DEC +03 01 MV = 3.69 FE/H = 0 R ------------------------------------------------------------------------ ( 25) GREENSTEIN, J.L., KEENAN, P.C. 1958: ASTROPHYS.J. 127, 172 ........................................................................ OBSERV. : PG, 4170-4410A, 2.8 OR 4.5 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 35 ATOMIC LINES, 25 FEATURES FROM CN, CH ANALYSIS: "MEAN" COG FROM WEHLAU (1956), T(SPECTR. TYPE), STANDARD STAR = MEAN OF: IOT GEM, KAP GEM, EPS VIR, ETA HER REMARKS : CN WEAK COMMENTS: CLASS : (D)A ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 219617 BD -14 6437 F8IV (SUBDWARF, WEAK METALS) AR 23 14.5 DEC -14 06 MV = 8.16 FE/H = --- (I) ------------------------------------------------------------------------ ( 38) ALLER, L.H., GREENSTEIN, J.L. 1960: ASTROPHYS.J.SUPPL. 5, 139 ........................................................................ OBSERV. : PG, 3650-4900A, 10 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 65: ANALYSIS: COG(THEOR.COG FROM WRUBEL 1949: AP.J. 109, 66), T(SOLAR EXC.TEMP. ASSUMED), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : D(T)AA, (I) ======================================================================== HD 219623 HR 8853 F7V AR 23 14.4 DEC +52 57 MV = 5.60 FE/H = 0 (R) ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 219978 BD +61 2423 K4.5IB AR 23 17.2 DEC +62 28 MV = 6.72 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 221148 HR 8924 K3III VAR (CN) AR 23 26.9 DEC -04 48 MV = 6.25 FE/H = 0 (L) ------------------------------------------------------------------------ (151) OINAS, V. 1974: ASTROPHYS.J.SUPPL. 27, 391 AND 405 ........................................................................ OBSERV. : PG, 5000-6820A, 6.7 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: DAOR ANALYSIS: LTE(ATLAS, UNBLANKET.), T(SCAN 5000-10800A, HALFA) G(IONIZATION), F-VALUES FE: DIFF(SUN), DAOR REMARKS : FINDS CORRELATION BETWEEN SPECTROSCOPIC GRAVITY AND TEMPERATURE (NEW OPACITY SOURCE?) COMMENTS: CLASS : DTGMAA, (L) ======================================================================== HD 221170 BD +29 4940 G2IV (WEAK METALS, EMISS H+K) AR 23 27.0 DEC +30 09 MV = 7.66 FE/H = ---- R ------------------------------------------------------------------------ ( 14) WALLERSTEIN, G., GREENSTEIN, J.L., PARKER, R., HELFER, H.L., ALLER, L.H. 1963: ASTROPHYS.J. 137, 280 ........................................................................ OBSERV. : PG, 5160-6260A, 15.3 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 120: ANALYSIS: COG, DIFF(SUN), T(LINE EXCITATION, GRI, IONIZATION) REMARKS : PRELIMINARY ANALYSIS COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 13.5+15.3 A/MM INSTRUM.: MT.PALOMAR 200-INCH, MT.WILSON 100-INCH, COUDE LINELIST: 50 ANALYSIS: COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), DIFF(SUN, EPS VIR), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (332) LUCK, R.E., BOND, H.E. 1981: ASTROPHYS.J. 244, 919 ........................................................................ OBSERV. : DATA FROM ( 14) WALLERSTEIN ET AL.1963: AP.J. 137, 280 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, LINES), G(FE I+II LINES), F-VALUES: DIFF(SUN) REMARKS : REANALYSIS COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, V-K, B-V), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 221345 14 AND G8III (EMISS H+K) AR 23 28.8 DEC +38 58 MV = 5.22 FE/H = 0 (I) ------------------------------------------------------------------------ ( 21) SCHWARZSCHILD, M., SCHWARZSCHILD, B., SEARLE, L., MELTZER, A. 1957: ASTROPHYS.J. 125, 123 ........................................................................ OBSERV. : PG, 4100-4500A, 10.2 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LL, 78, GIVE CENTRAL LINE DEPTHS ANALYSIS: COG, DIFF(SUN) REMARKS : COG SHIFTS RELATIVE TO SUN WERE DERIVED BY 15 FE II LINES COMMENTS: CLASS : (D)AA, (I) ======================================================================== HD 221377 BD +51 3630 F7VM (WEAK METALS) AR 23 28.9 DEC +52 08 MV = 7.57 FE/H = -- (R?) ------------------------------------------------------------------------ (302) SNEDEN, C., LAMBERT, D.L., WHITAKER, R.W. 1979: ASTROPHYS.J. 234, 964 ........................................................................ OBSERV. : PG, ???? , 9 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: DAOR ANALYSIS: LTE(PEYTREMANN 1974?), T(B-Y, FE I EXCITATION), G(FE, CR, TI, V IONIZATION), F-VALUES: DIFF(SUN)? REMARKS : COMMENTS: THIS PAPER DEALS WITH THE DERIVATION OF O ABUNDANCES ONLY. IT BRIEFLY RELATES THE FULL ANALYSIS THE RESULTS OF WHICH ARE QUOTED: TEFF, G, MICRO, FE/H CLASS : DTGMA, (R?) ======================================================================== HD 222107 LAM AND G8III (EMISS H+K) AR 23 35.1 DEC +46 11 MV = 3.82 FE/H = -- (L) ------------------------------------------------------------------------ ( 43) HELFER, H.L., WALLERSTEIN, G. 1968: ASTROPHYS.J.SUPPL. 16, 1 ........................................................................ OBSERV. : PG, 5100-6340A, 6.6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 250: ANALYSIS: COG, DIFF(GAM TAU), T(UBVGRI) REMARKS : COMMENTS: CLASS : DTAA, (L) ======================================================================== HD 222368 IOT PSC F7V AR 23 37.4 DEC +05 21 MV = 4.13 FE/H = - R ------------------------------------------------------------------------ ( 75) POWELL, A.L.T. 1970: MONTHLY NOTICES ROY.ASTRON.SOC. 148, 477 ........................................................................ OBSERV. : PG, 3600-4750A, 10 A/MM INSTRUM.: RGO 30-INCH, COUDE, LINELIST: 140:, LLWW: POWELL 1971: ROY.OBS.BULL. 167 ANALYSIS: COG, DIFF(SUN), T(GRI, BETA-INDEX, (HGAMMA PROFILE)) PE(IONIZATION TI, FE, CR) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I, BETA), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ======================================================================== HD 222404 GAM CEP K1IV (EMISS H+K+MG(UV), CN) AR 23 37.3 DEC +77 21 MV = 3.21 FE/H = 0 R? ------------------------------------------------------------------------ (126) BAKOS, G.A. 1971: J.ROY.ASTRON.SOC.CAN. 65, 222 ........................................................................ OBSERV. : PG, 3900-4600A, 12 A/MM INSTRUM.: D.DUNLAP OBS. 74-INCH LINELIST: 200 ANALYSIS: COG, T(LINE EXCIT.), PE(IONIZATION) F-VALUES FROM CORLISS, WARNER 1964: AP.J.SUPPL. 8, 395 REMARKS : THEORET. COG FROM UNSOELD 1968: STERNATMOSPHAEREN COMMENTS: CLASS : (T)AA ------------------------------------------------------------------------ (139) GLEBOCKI, R. 1972: ACT.ASTRON. 22, 141 ........................................................................ OBSERV. : PG, 5200-6400A, 20 A/MM INSTRUM.: LOVELL 72-INCH, CASSEGRAIN LINELIST: 82, LLWW: GLEBOCKI, STROBEL 1970: ACT.ASTRON. 20, 361 ANALYSIS: COG, DIFF(EPS VIR), T(FE I EXCITATION) REMARKS : DERIVES FE/H ABUNDANCES ONLY COMMENTS: CLASS : DTA, L ------------------------------------------------------------------------ (356) GRATTON, L., GAUDENZI, S., ROSSI, C., GRATTON, R.G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 201, 807 ........................................................................ OBSERV. : PG, 3980-4800A, 3.15 A/MM INSTRUM.: OHP 1.9M, COUDE LINELIST: LW, 180: ANALYSIS: LTE(GUSTAFSSON), T(THEOR./EMPIR. COG, EXCIT.TEMP.) G(TI I/II IONIZATION) F-VALUES: VARIOUS SOURCES (1962-1979) REMARKS : DERIVE FE AND TI ABUNDANCES ONLY COMMENTS: CLASS : TGMA, R ------------------------------------------------------------------------ (351) LAMBERT, D.L., RIES, L.M. 1981: ASTROPHYS.J. 248, 228 ........................................................................ OBSERV. : PE, RETICON, 5086, 5135, 4835, 6300, 6363A, 0.05A DATA ON CN FROM LITERATURE INSTRUM.: MCDONALD 2.7M, COUDE LINELIST: LW, 5 ANALYSIS: LTE(GUSTAFSSON, ATLAS), ATOMIC+MOLEC. LINE BLANKETING, T+G(RIES 1981 -TO BE PUBL.- : T(FE I EXCITATION), G(FE I/II IONIZATION) ) F-VALUES: C2, OI: EXPERIM.+THEOR., CN: SOLAR REMARKS : DERIVE ABUNDANCES FOR C, N, O ONLY COMMENTS: CF. LAMBERT, RIES 1977: AP.J. 217, 508 CLASS : (D)MA, R? ------------------------------------------------------------------------ (A28) GRATTON, R.G. 1983: MONTHLY NOTICES ROY.ASTRON.SOC. 202, 231 ........................................................................ OBSERV. : DATA FROM (356) GRATTON ET AL.1982: MNRAS 201, 807 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), DIFF(SUN), T+G(FROM (356)), FE/H FROM 6 STRONG FE I LINES REMARKS : COMMENTS: CLASS : DMA, L ======================================================================== HD 222574 104 AQR G0IAB: AR 23 39.2 DEC -18 06 MV = 4.82 FE/H = 0 (R) ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 223047 PSI AND G5IB+... (EMISS H+K) AR 23 43.5 DEC +46 09 MV = 4.95 FE/H = 0 R ------------------------------------------------------------------------ (264) LUCK, R.E. 1977: ASTROPHYS.J. 212, 743 ........................................................................ OBSERV. : PG, 5100-6800A:, 3.5-7.5 A/MM INSTRUM.: MCDONALD 2.1M, COUDE LINELIST: LESS THAN 800 ANALYSIS: COG, DIFF(EPS VIR, EPS GEM), THEOR.COG FROM LTE MODELS(GUSTAFSSON), T(FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE) REMARKS : COMMENTS: CLASS : DTGMAA, R ------------------------------------------------------------------------ (388) LUCK, R.E. 1982: ASTROPHYS.J. 256, 177 ........................................................................ OBSERV. : DATA FROM LUCK 1977: ASTROPHYS.J. 212, 743 AND 218, 752 INSTRUM.: LINELIST: ANALYSIS: LTE(GUSTAFSSON), T+G(FE I, II LINES) F-VALUES: DIFF(SUN) REMARKS : USES ONLY LINES WITH EQ.WIDTH LESS THAN 200MA COMMENTS: DERIVES FE ABUNDANCE ONLY CLASS : DTGMSA, R ======================================================================== HD 223385 6 CAS A3IAE (COMPOSITE) AR 23 46.4 DEC +61 56 MV = 5.43 FE/H = ? (L) ------------------------------------------------------------------------ (172) AYDIN, C. 1972: ASTRON.ASTROPHYS. 19, 369 ........................................................................ OBSERV. : PG, 3710-4860A, 12.4 A/MM INSTRUM.: OHP 1.5M, 1.9M, COUDE LINELIST: 280:, LLWW: AYDIN 1972: ASTRON.ASTROPHYS.SUPPL. 7, 331 ANALYSIS: COG, DIFF(ALF CYG), T+G(HBETA, HGAMMA, BALMER DISC.), PE(FE I/II IONIZATION, INGLIS-TELLER) F-VALUES: CORLISS, WARNER 1964 REMARKS : DERIVES FE, TI, CR ABUNDANCES ONLY COMMENTS: CLASS : DTGA, (L) ======================================================================== HD 224165 HR 9053 G8IB AR 23 53.0 DEC +47 05 MV = 6.00 FE/H = 0 (R) ------------------------------------------------------------------------ (A06) LUCK, R.E. 1982: ASTROPHYS.J. 263, 215 ........................................................................ OBSERV. : PG, 4950-6900A, 0.1 A, S/N= 30 INSTRUM.: KPNO 4M, ECHELLE LINELIST: 300-600, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION), F-VALUES: DIFF(SUN, HOLWEGER MODEL) REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 224635/6 HR 9074/5 G0V AR 23 56.9 DEC +33 27 MV = 6.60 FE/H = 0 (R) ------------------------------------------------------------------------ ( 62) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 36, 191 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(BETA) G(PARALL. + EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : BOTH BINARY COMPONENTS ASSUMED TO BE IDENTICAL, EXTENSION OF HEARNSHAW 1974: ASTRON.ASTROPHYS. 34, 263 COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, (R) ======================================================================== HD 224930 85 PEG G5VB (EMISS H+K) AR 23 59.6 DEC +26 49 MV = 5.75 FE/H = -- R ------------------------------------------------------------------------ ( 40) WALLERSTEIN, G., HELFER, H.L. 1959: ASTROPHYS.J. 129, 720 ........................................................................ OBSERV. : PG, 5150-6270A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 120:, LLWW: WALLERSTEIN, HELFER 1959: AP.J. 129, 347 ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : COMMENTS: CLASS : DTGAA ------------------------------------------------------------------------ ( 29) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1960: ASTROPHYS.J. 132, 553 ........................................................................ OBSERV. : DATA FROM ( 28) WALLERSTEIN ET AL.1959: AP.J. 129, 347 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(FE I EXCITATION), PE(IONIZATION FE, CR) REMARKS : REANALYSIS, BECAUSE A SMALL TERM IN SAHA'S EQUATION HAD BEEN NEGLECTED IN ( 40) WALLERSTEIN, HELFER 1959: AP.J. 129, 720 COMMENTS: CLASS : DTGAA ------------------------------------------------------------------------ ( 3) WALLERSTEIN, G. 1962: ASTROPHYS.J.SUPPL. 6, 407 ........................................................................ OBSERV. : PG, 5210-6265A, 15 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 135, LLWW: WALLERSTEIN, HELFER 1959: AP.J. 129, 347 ANALYSIS: COG, DIFF(SUN), T(B-V, G-R, LINE EXCITATION) REMARKS : COMMENTS: CLASS : DTAA ------------------------------------------------------------------------ ( 37) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1963: ASTROPHYS.J. 138, 97 ........................................................................ OBSERV. : PG, 4000-4770A, 4.5 A/MM; 5120-6280A, 6 A/MM INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: LLWW, 320: ANALYSIS: COG, DIFF(SUN), EMPIRICAL COG FROM FE I, T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ ( 85) ALEXANDER, J.B. 1967: MONTHLY NOTICES ROY.ASTRON.SOC. 137, 41 ........................................................................ OBSERV. : WALLERSTEIN 1962: AP.J.SUPPL. 6, 407 INSTRUM.: LINELIST: ANALYSIS: COG, DIFF(SUN), T(COMP. OF FE I LINES WITH SOLAR COG FROM COWLEY, COWLEY 1964: AP.J. 140, 713; A PE-DEPENDENT CORRECTION IS APPLIED WHICH HAD BEEN DERIVED FROM MODELS OF CAYREL, JUGAKU 1963: ANN.ASTROPHYS. 26, 495) REMARKS : COMMENTS: CLASS : DTA, L ------------------------------------------------------------------------ ( 61) HEARNSHAW, J.B. 1974: ASTRON.ASTROPHYS. 34, 263 ........................................................................ OBSERV. : PG, 4150-4800A, 7 A/MM INSTRUM.: OHP 1.5M, COUDE LINELIST: 120, LLWW: HEARNSHAW 1975: ASTRON.ASTROPHYS.SUPPL. 19, 321 ANALYSIS: LTE(PEYTREMANN), T(R-I), G(EVOL. TRACKS) FE+CH: DIFF(SUN) REMARKS : COMMENTS: DERIVES FE AND CH ABUND. ONLY CLASS : DT(G)MA, R ------------------------------------------------------------------------ (304) CLEGG, R.E.S 1977: MONTHLY NOTICES ROY.ASTRON.SOC. 181, 1 ........................................................................ OBSERV. : PG, 3800-4700A, 13 A/MM INSTRUM.: KPNO 36-INCH, COUDE LINELIST: ANALYSIS: DIFF(SUN), LTE(GUSTAFSSON) T(BETA, R-I, B-V, B-Y) G(UVBY-BETA, MASS+TRIG.PARALLAX) F-VALUES: NH, CN, CH DIFF(SUN) SPECTRUM SYNTHESIS OF MOLECULAR BANDS REMARKS : COMMENTS: CLASS : DTGMSA, R ------------------------------------------------------------------------ (A24) CLEGG, R.E.S., LAMBERT, D.L., TOMKIN, J. 1981: ASTROPHYS.J. 250, 262 ........................................................................ OBSERV. : PE, 100A SECTIONS AT 6600, 7100, 8300, 9300 A, 0.2 A 30 A SECTIONS AT 6160, 6300, 8680, 8730 A, 0.1 A 20-30 A SECTIONS AT 4230, 4370, 5140, 8060 A, 0.1 A 100 A SECTIONS AT 5655, 5775, 6190 A, 0.2 A (FE I LINES) INSTRUM.: MCDONALD 2.7M, COUDE, ECHELLE, RETICON LINELIST: LW, LESS THAN 50:, PLUS 30 FE I LINES (DAOR) ANALYSIS: LTE(SCALED SOLAR MODELS(HOLWEGER MUELLER)), DIFF(SUN), T(V-R, V-I, BETA, UVBY; FE I EXCITATION), G(ABS.MAG.+MAIN SEQ.MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, R ======================================================================== HD 225212 3 CET K3IAB: AR 00 01.9 DEC -10 47 MV = 4.94 FE/H = 0 R ------------------------------------------------------------------------ (132) VAN PARADIJS, J. 1973: ASTRON.ASTROPHYS. 23, 369 ........................................................................ OBSERV. : PG, 5000-6650A, 6.5 A/MM INSTRUM.: MT.WILSON 100-INCH LINELIST: 800:, VAN PARADIJS 1973: A+A SUPPL. 11, 25 ANALYSIS: LTE(CARBON, GINGERICH 1969, EXTRAPOLATED), T(VRIJK, FE I EXCITATION), G(IONIZATION SC, TI, V, CR, FE), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ------------------------------------------------------------------------ (329) LUCK, R.E., BOND, H.E. 1980: ASTROPHYS.J. 241, 218 ........................................................................ OBSERV. : PE, RETICON, 175A SECTIONS CENTERED AT 6350, 6560, 6710A 0.3A, S/N= MORE THAN 50 INSTRUM.: MT.WILSON 100-INCH, COUDE LINELIST: 175-250, DAOR ANALYSIS: LTE(GUSTAFSSON), T(FE I EXCITATION), G(FE I/II IONIZATION) F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DTGMAA, L ======================================================================== HD 225239 HR 9107 G2V AR 00 02.3 DEC +34 23 MV = 6.10 FE/H = - (L) ------------------------------------------------------------------------ (385) SPITE, F., SPITE, M. 1982: ASTRON.ASTROPHYS. 115, 357 ........................................................................ OBSERV. : 6600-6740A, 4.7 A/MM, 0.26 A, S/N= 100 INSTRUM.: CFH 3.6M, COUDE, RETICON LINELIST: ANALYSIS: LTE(PEYTREMANN 1974), T+G(CARNEY 1982: AP.J. 233, 211) REMARKS : GIVE FE/H ABUNDANCE ONLY COMMENTS: CLASS : MA, (L) ======================================================================== HD 232078 BD +16 3924 K3IIP AR 19 35.9 DEC +16 42 MV = 8.70 FE/H = --- R ------------------------------------------------------------------------ ( 1) HELFER, H.L., WALLERSTEIN, G., GREENSTEIN, J.L. 1959: ASTROPHYS.J. 129, 700 ........................................................................ OBSERV. : PG, 4000-4900A, 9+18 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE LINELIST: LLWW, 200: ANALYSIS: COG(WRUBEL 1949), DIFF(SUN), T(FE I EXCITATION) REMARKS : COMMENTS: CLASS : DTAA, L ------------------------------------------------------------------------ (350) LEEP, E.M., WALLERSTEIN, G. 1981: MONTHLY NOTICES ROY.ASTRON.SOC. 196, 543 ........................................................................ OBSERV. : PG, ???? , 6.8+13.5 A/MM INSTRUM.: MT.PALOMAR 200-INCH, COUDE, IT LINELIST: 98 ANALYSIS: DIFF(SUN, EPS VIR), COG(THEOR.COG FROM LTE(GUSTAFSSON) MODELS), T(B-V, V-K, FE I EXCITATION), G(FE I/II IONIZATION) REMARKS : COMMENTS: CLASS : DTGMAA, R ======================================================================== HD 233666 BD +54 1323 G2WE (WEAK METALS) AR 09 38.9 DEC +53 42 MV = 9.31 FE/H = --- (R) ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, V-K), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MAA, (R) ======================================================================== HD 233891 BD +52 1601 G5III (WEAK METALS) AR 11 57.4 DEC +52 03 MV = 8.80 FE/H = --- R ------------------------------------------------------------------------ (296) SNEDEN, C. 1974: ASTROPHYS.J 189, 493 ........................................................................ OBSERV. : PG, 3800-4700A, 18 A/MM INSTRUM.: MCDONALD 2M, COUDE LINELIST: ANALYSIS: SPECTR.SYNTHESIS, LTE(ATLAS) T(EXCITATION), G(IONIZATION) F-VALUES CHECKED WITH SOLAR SPECTRUM REMARKS : DERIVES C,N ABUNDANCES, ESTIMATES O COMMENTS: NO PHOTOMETRIC INFORMATION WAS USED CLASS : (D)TGMSA, R ------------------------------------------------------------------------ (A21) GRATTON, R.G., ORTOLANI, S. 1984: ASTRON.ASTROPHYS. 137, 6 ........................................................................ OBSERV. : PG, 5680-6450A, 10 A/MM, 0.3 A, S/N= 20..30 INSTRUM.: ASIAGO 1.8M, CASSEGRAIN, ECHELLE, IT LINELIST: LW, LESS THAN 90: ANALYSIS: LTE(GUSTAFSSON), T(B-Y, V-K), G(ABS.MAG.+ASSUMED MASS), F-VALUES: DIFF(SUN) REMARKS : COMMENTS: CLASS : DT(G)MA, R ======================================================================== HD 237846 BD +58 1218 F8 AR 09 49.1 DEC +58 09 MV = 10.3 FE/H = ---- (R) ------------------------------------------------------------------------ (A07) LUCK, R.E., BOND, H.E. 1985: ASTROPHYS.J. 292, 559 ........................................................................ OBSERV. : PG, IT, 3800-6800A, 4.6 A/MM, 0.2A INSTRUM.: KPNO 4M, ECHELLE LINELIST: 500:, LLWW: LUCK, BOND 1985: AP.J.SUPPL. 59, 249 ANALYSIS: LTE(GUSTAFSSON), T(B-Y, FEI EXCITATION) G(FEI/II IONIZATION), F-VALUES DIFF(SUN) SEE LUCK, BOND 1981: AP.J. 244, 919 REMARKS : COMMENTS: CLASS : DTGMAA, (R) ======================================================================== HD 268757 RMC 59 G8... AR 04 54.4 DEC -69 17 MV = 10.15 FE/H = 0 (R) ------------------------------------------------------------------------ (240) FRY, M.A., ALLER, L.H. 1975: ASTROPHYS.J.SUPPL. 29, 55 ........................................................................ OBSERV. : PG, 3960-6610A, 4-16 A/MM INSTRUM.: LICK 120-INCH, COUDE LINELIST: LLWW, 560: ANALYSIS: LTE(CARBON, GINGERICH 1969 ?), SPECTRUM SYNTHESIS, T(FE I, CR I, TI I EXCITATION), G(FE I/II, CR I/II IONIZATION), F-VALUES: VARIOUS SOURCES AS LISTED REMARKS : COMMENTS: CLASS : DTGMSAA, (R) ======================================================================== HD 274939 CD -48 1866 G0 (WEAK METALS) AR 05 32.0 DEC -47 58 MV = 9.42 FE/H = --- (R) ------------------------------------------------------------------------ (414) GRATTON, R.G. 1983: ASTRON.ASTROPHYS. 123, 289 ........................................................................ OBSERV. : PG, IT, 4860-6600A, 5 A/MM INSTRUM.: CTIO 4M, R-C LINELIST: LLWW, 180: ANALYSIS: LTE(GUSTAFSSON), T(V-K), G(IONIZATION FE,TI,SC,CR,Y) F-VALUES: DIFF(SUN) REMARKS : GRAVITIES UNCERTAIN COMMENTS: CLASS : DTGMAA, (R)