02366+1226 = HR 763 = McA 7: These three measurements of 31 Ari were based 02366+1226 on reprocessing of archival video data. A combined 02366+1226 spectroscopic/speckle orbital analysis of this very close system is 02366+1226 now in progress, in collaboration with Frank Fekel. 04404+1631 = vB 185 = CHARA 154: This confirms the discovery observation of 04404+1631 this Hyades binary, made in 1991 (Mason et al. 1993AJ....105..220M). 05271+1758 = ADS 4038 = McA 19 Aa: All archival data for this system were 05271+1758 reprocessed, resulting in four new unresolved measures as well as 05271+1758 the new 1991 measurement. In addition, new rho and theta values have 05271+1758 been determined for the observations originally published from 05271+1758 1986.9-1988.3 (McAlister et al., 1989AJ.....97..510M), 1988.7-1989.2 05271+1758 (McAlister et al., 1990AJ.....99..965M), and 1990.3-1990.8 05271+1758 (Hartkopf et al., 1992AJ....103.1976H). The date of the 1988.2518 05271+1758 measurement was incorrectly given as 1988.2490 in McAlister et al. 05271+1758 (1989AJ.....97..510M). Orbital analysis of this system is in 05271+1758 progress; a preliminary orbit gives a period of ~15.3 years and a 05271+1758 semi-major axis of 0.080". 06017+2224 = HR 2116 = CHARA 161: This confirms the discovery observation, 06017+2224 made in 1988 (McAlister et al., 1993, Cat. ). 06212+2932 = HR 2272 = CHARA 165: This confirms the discovery observation, 06212+2932 made in 1988 (McAlister et al., 1993, Cat. ). 07277+2127 = ADS 6089 = McA 30 Aa: A combined spectroscopic/speckle orbit of 07277+2127 this system has been undertaken in collaboration with Frank Fekel. 08095+3213 = ADS 6623 = CHARA 190 Aa: This is a new component to the wide 08095+3213 (2.8") pair STF 1187, discovered by Struve in 1829. 10453+3831 = ADS 7915 = Ho 532 AB and CHARA 191 Aa: The Aa pair appears to be 10453+3831 a new component to the 0.7" pair Ho 532. This new component was 10453+3831 actually first resolved back in 1983 (McAlister et al., 10453+3831 1987AJ.....93..688M) but it was believed at the time that the 10453+3831 measurement was of the known pair (the wide component laid outside 10453+3831 the processor "window" of our old autocorrelator). Reprocessing 10453+3831 of our archival video data allowed us to resolve both components in 10453+3831 the 1983 and 1984 data sets, although both early measurements of 10453+3831 the Aa component are quite weak. 11150+3735 = ADS 8102 = CHARA 192 Aa: This is a new component to the 0.6" pair 11150+3735 STT 232, discovered by Otto Struve in 1843. Reprocessing of archival 11150+3735 data (whose 1987 and 1988 measurements for the wide pair were 11150+3735 originally published in McAlister et al., 1989AJ.....97..510M) has 11150+3735 allowed us to confirm this discovery and also to note that the 11150+3735 system appears to be accelerating toward periastron. 11182+3132 = ADS 8119 = STF 1523 AB: An orbital analysis of Xi UMa, including 11182+3132 both the AB pair, the astrometric companion, and the 11182+3132 newly-discovered Bc companion, is now in preparation by Mason et al. 13175-0041 = HR 5014 = Fin 350: Orbital analysis of this system is in progress. 13175-0041 In the process we have been able to resolve the uncertainty between 13175-0041 a possible short-period/high-eccentricity orbit and a 13175-0041 long-period/low-eccentricity one. 13197+4747 = ADS 8862 = CHARA 193 Aa: This is a new component to the 1.5" 13197+4747 49-year period pair of M2 dwarfs Hu 644. This is the only one of the 13197+4747 current crop of new interferometric binaries which has not yet been 13197+4747 confirmed. 15245+3723 = ADS 9626 = CHARA 181 Aa: This confirms the discovery observation 15245+3723 of this pair, made in 1988 (McAlister et al. 1993, 15245+3723 Cat. ). 17215+2845 = HR 6466 = CHARA 194 Aa: This is a new close companion to the 0.7" 17215+2845 pair Kui 80. The primary of this system is listed in the preliminary 17215+2845 version of the BSC5 (Hoffleit & Warren, 1992, Cat. ) as a 17215+2845 G0III spectroscopic binary. 17217+3958 = HR 6469 = McA 47: A new combined spectroscopic/interferometric 17217+3958 orbital solution has now been completed and submitted to AJ 17217+3958 (Scarfe et al., 1994AJ....107.1529S). 17572+2400 = HR 6697 = McA 50: All our CCD speckle data for this close system 17572+2400 have been reprocessed and examined. In addition, we have listed 7 17572+2400 negative measures dating from observations made at the KPNO 2.1-m 17572+2400 in the 1970's. A combined spectroscopic/interferometric orbit is now 17572+2400 in preparation (McAlister et al. 1994). 17584+0427 = +04 3562 = Kui 84: A measurement published by McAlister et al. 17584+0427 (1987AJ.....93..688M) dating from 1985.4872 was misidentified as 17584+0427 being of Kui 84; the measurement actually was of Kui 89 17584+0427 (WDS 18594-1250). In addition, an observation of Kui 84 dating from 17584+0427 1988.6655 (theta=270.6{deg}, rho=0.134") was published by McAlister 17584+0427 et al. (1990AJ.....99..965M). These data have been reprocessed, 17584+0427 and we now believe this measurement was spurious. 18594-1250 = HR 7166 = Kui 89: This measurement was incorrectly attributed to 18594-1250 Kui 84 (WDS 17584+0427) by McAlister et al. (1987AJ.....93..688M). 20158+2749 = HR 7744 = CHARA 94 Aa: These two observations confirm the discovery 20158+2749 measurement of this close component, made in 1985 (McAlister et al. 20158+2749 1987AJ.....93..688M), and indicate considerable motion during this 20158+2749 interval. 20462+3358 = ADS 14274 = CHARA 100 Aa: This appears to have finally confirmed 20462+3358 the discovery observation of this component, made in 1983 20462+3358 (McAlister et al. 1987AJ.....93..688M). A number of unresolved 20462+3358 observations of this very close system, dating from 1979 to 1981, 20462+3358 were published by Hartkopf & McAlister (1984PASP...96..105H). 20474+3629 = ADS 14296 = McA 63 Aa: Orbital analysis of Lambda Cyg is in 20474+3629 preparation; a preliminary orbit gives a period of 11.8 years and a 20474+3629 semi-major axis of 0.049". 21145+1001 = ADS 14773 = STT 535 AB: A combined spectroscopic/speckle orbit of 21145+1001 this system has been undertaken in collaboration with Frank Fekel. 23460+4625 = HR 9003 = McA 75 Aac: With this measurement we appear to have 23460+4625 finally confirmed the discovery observation of this component, made 23460+4625 in 1981! (McAlister et al. 1984ApJS...54..251M).