%----------------------------------------------------------------------
% Title:  A catalogue of high-mass X-ray binaries (4nd edition)
% Source: E:\API\catalog\hmxb.tex
% Original Author:            Qingzhong LIU <qliu@science.uva.nl or qzliu@pmo.ac.cn>
% Created:                    May 24, 2005
% First version:              QZL, Nov. 16, 2005
% commented    :              Marc Rib\'o, Nov. 25, 2005
% Revised      :              EDVDH Dec. 16, 2005
% commented    :              Sylvain Chaty, Dec. 18, 2005
% commented    :              Ignacio Negueruela, Feb 16, 2006
% Final version:              QZL Dec. 30, 2005
% Submitted  :                Jan. 23, 2006
% Basically accepted :        March 4, 2006
% resubmitted  :              Apr. 17, 2006
% accepted     :              Apr. 21, 2006
% second post-proof revision; QZL, October  2006


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\begin{document}
%\headnote{Research Note}


Reference number: AA/2006/4987

Title: Catalogue of high-mass X-ray binaries in the Galaxy ($4^{th}$ edition)

Authors: Q.Z. Liu, J. van Paradijs, and E.P.J. van den Heuvel

Name of the journal, year, volume and first page: A\&A, 2006, ??, ??

Keywords: Catalog - X-ray: binaries - Stars: emission-line, Be - Stars: binaries: close

Description of the table and its columns:

Table 1 lists the 114 HMXB candidates in the Galaxy. The format of Table 1 is similar to the previous edition and
almost the same with the HMXB catalogue in the Magellanic Clouds (Liu, van Paradijs \& van den Heuvel 2000; 2005), of
which the present catalogue is meant to be an update. If there is any doubt about an entry, a question mark follows the
item. In the table the sources are ordered according to the right ascension of sources; part of the (mainly numerical)
information on a source is arranged in six columns, below which additional information is provided for each source in
the form of key words with reference numbers [in square brackets]. The columns have been arranged as follows.

In Column 1 the first line contains the source name, with rough information on its sky location, according to the
conventional source nomenclature of space experiments in which the source was detected, hhmm$\pm$ddd or
hhmm.m$\pm$ddmm. Here hh, mm, and ss indicate the hours, minutes and seconds of right ascension, ddd the declination in
units of 0.1 degree (in a small number of cases, the coordinates shown in the name are given with more, or fewer,
digits). The prefix J indicates a name based on J2000 coordinates. Otherwise, 1950 coordinates were used in the name.
An alternative source name is given in the second line. In the third line of Column
1, the source types are indicated with a letter code, as follows:\\
\\
$\bullet$ P: X-ray pulsar (66);\\
$\bullet$ T: transient X-ray source (62);\\
$\bullet$ E: eclipsing system (9);\\
$\bullet$ R: radio emitting HMXBs (9);\\
$\bullet$ C: cyclotron resonance scattering feature at X-ray

~~spectrum (16);\\
$\bullet$ U: ultra-soft X-ray spectrum (1). These sources include

~~black-hole candidates (BHC); some $`$extreme ultra-

~~soft$'$ (EUS) source may be a white dwarf (WD) on

~~whose surface steady nuclear burning takes place.\\

Column 2 contains the right ascension (RA) and declination (DEC) of the source for equinox J2000.0 in the first two
lines. RA is given as hhmmss.s to an accuracy of 0.1 s, DEC is given in $^\circ$ ' ", to an accuracy of 1" (in a small
number of cases, the coordinates are given with more, or fewer, digits). The third line gives the galactic longitude
and latitude to an accuracy of 0.1$^\circ$ (except for sources close to the galactic center, where these coordinates
are given to 0.01$^\circ$). A reference for the source position is given below the columnar information under $'pos.'$.
In the parentheses following the $'pos.'$, we provide some information on the type of observation from which the source
position has been derived. The following abbreviations are used: o, optical; x, X-ray; r, radio; IR, infrared.
Following the type of observation, we give an indication of the accuracy of this position, in the form of equivalent
(90 percent confidence level) error radii, but in several cases this can only be considered an approximation (e.g. when
the error box is not circular). When no accuracy is quoted, it is about one arcsecond or better.

The first and second lines of Column 3 give the names of the optical counterpart to an X-ray source. The third line
contains a reference to a finding chart. An asterisk followed by a number or letter refers to the star number used in
the finding chart; "star" refers to a star in the finding chart that has not been assigned a number or letter. Many
optical counterparts have been indicated with a variable-star name, as given in the
$General~Catalogue~of~Variable~Stars$ and in recent name lists of variable stars as published regularly in the
$IAU~Information~Bulletin~on~Variable~Stars$, or a number in a
well-known catalogue (e.g., HD, SAO, GSC, 2MASS). %For X-ray sources in globular clusters, the
%cluster name is here given, in addition to the name of a stellar optical counterpart.

The fourth column contains some photometric information on the optical counterpart. In the first line, the apparent
visual magnitude, $V$, and the color indices $B-V$ and $U-B$ are listed. The second line contains the spectral type of
the optical counterpart and an estimate of the interstellar reddening, $E_{B-V}$.

The fifth column lists the near-infrared magnitudes at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns),
detected with the Two Micron All Sky Survey (2MASS)(Skrutskie et al. 2006).

In Column 6, the maximum X-ray flux, or the range of observed X-ray fluxes (2--10 keV, unless otherwise indicated), is
given in units of
\begin{eqnarray*}
1\mu Jy & = &10^{-29}~ erg~ cm^{-2}~ s^{-1} Hz^{-1}\\
       & = & 2.4\times 10^{-12}~ erg~  cm^{-2}~  s^{-1}~ keV^{-1}.
\end{eqnarray*}

%1 mCrab= 1.4x10^{-11} erg/s/cm2 for a source with a Crab-like spectrum.

The first line in Column 7 gives the orbital period in days. The second line contains the pulse period for X-ray
pulsars, in seconds. The third line contains a reference in which the orbital and/or pulse periods were detected.



\begin{table*}[t]
\caption{High-mass X-ray binaries in the Galaxy}
\begin{tabular}{p{3.6cm}p{1.9cm}p{2.3cm}p{3.3cm}p{0.8cm}p{1.9cm}p{1.7cm}}
%\noalign{\smallskip}
\hline \noalign{\smallskip}
%\multicolumn{7}{p{17.6cm}}{Table 3.  (continued) }\\
%\hline \noalign{\smallskip}
Name(s)  & RA (J2000)       & Opt. Ctp. & V, $B-V$, $U-B$     & J & F$_{x}$ & P$_{orb}$(d)   \\
         & DEC (J2000)      &           & Sp. type, E$_{B-V}$ & H & $\mu$Jy & P$_{pulse}$(s) \\
type     & $l^{II}, b^{II}$ & [FC]      &                     & K &         &                \\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J00370+6122       & 00 37 10      & BD +60 73     & 9.65, 0.56,       & 8.389 & 8           & 15.665 \\
1RXS J003709.6+612131 & +61 21 35     & LS I +61 161  & B0.5II--III, 0.75 & 8.265 & (2--28 keV) &       \\
                      & 121.2, $-$1.5 &               & [640]             & 8.166 & [165]       & [165] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [640]; distance of 3.0 kpc: [640]; variable hard X-ray source: [165]; no radio
emission detected: [75].
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
2S 0053+604    & 00 56 42.5    & $\gamma$ Cas & 1.6--3.0, $-$0.15, $-$1.08 & 2.039 & 5--11  & 203.59  \\
3A 0053+604    & +60 43 00     &              & B0.5 Ve, 0.05              & 1.993 &        &         \\
R              & 123.6, $-$2.1 & [175]        & [528]                      & 1.756 & [64]   & [279] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; X-ray spectrum: [220, 545, 588]; UV observations: [169, 275, 286, 759];
variable Be star: [469, 810]; radial-velocity variations: [358]; $v_rsin i \sim$ 300--500 \kms: [312, 318, 528]; system
velocity: [795]; radio/mm obs.: [178, 817]; polarimetry: [107]; optical interferometry H$\alpha$ envelope: [542, 763];
non-radial pulsations: [855]; wind structure: [816]; a WD sys.: [263]; multiwavelength (mwl) obs.: [305, 716]; ISO spe.
and envelope structure: [304]; secondary mass of $\sim$1\msun: [279]; $e=0.26$: [279]; X-ray and optical variations:
[664]; multi-component of X-ray emission: [717]; distance of 0.19 kpc: [598].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
2S 0114+650  & 01 18 02.7   & V662 Cas            & 11.0, 1.2, 0.1  & 8.597 & 4     & 11.6       \\
             & +65 17 30    & LS I +65$^\circ$010 & B0.5 Ib, 1.4    & 8.296 &       & 10008      \\
P, C?        & 125.7, +2.6  & [175]               & [2, 148]        & 8.107 & [64]  & [148, 210] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [598]; X rays: [210, 211, 391, 486]; opt. spectra: [2, 148, 434]; $v_rsin i
\sim$ 45 \kms: [2]; opt. polarimetry: [41]; magnetar origin: [430]; astrophys. parameters: [633]; opt. photometry:
[758]; superorbital period of 30.7 d: [194]; distance of 7.2 kpc: [633]; spin-up: [55]; likely a cyclotron resonance
scattering feature at 22 keV with one harmonic (implying a magnetic field of 2.5$\times$10$^{12}$ G)
[55], but not detected with SAX: [486]. %no radio emission detected: [Nelson \& Spencer 1988]
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
4U 0115+634   & 01 18 31.9   & V635 Cas  & 14.5--16.3, 1.4, 0.3 & 11.622 & $<$2--350 & 24.3       \\
4U 0115+63    & +63 44 24    &           & B0.2Ve, 1.5          & 11.023 &           & 3.61       \\
T, P, C       & 125.6, +1.0  & [361]     & [507, 554, 784]      & 10.629 & [64]      & [547, 625] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [361]; X-ray outbursts: [614, 659, 675, 750, 776]; recurrence time 3 yr (?):
[831]; rapid X-ray variation: [77]; X-ray spectrum: [659, 830]; X-ray cyclotron lines: [282, 549, 750]; opt.
pre-outburst behavior: [407, 507]; long-term opt. phot.: [507]; opt. spectra: [317, 784]; $v_rsin i \sim 365 km/s$:
[317]; mwl obs. during an outburst: [557]; distance of 7--8 kpc: [554]; $e=0.34$: [625]; QPOs during outburst: [110,
721].
% (xxx ????In 1990, two harmonic cyclotron features were
%detected at energies of 11.3 and 22.1 keV, in agreement with previous observations. In 1991,
%the structure changed to a single absorption at an energy of 15.6 keV, which is interpreted as
%the fundamental resonance: [G011]. cyclotron absorption features: [G012]; two cyclotron
%absorption features at 15 and 23 keV: [IAUC 7482];)
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J01363+6610 & 01 35 50    & EM* GGR 212 & 13.29, 1.39,   & 10.039 & 9            &  \\
                & 66 12 40    &             & B1Ve, 1.61     & 9.565  & (17--45 keV) &  \\
T               & 127.4, 3.7  & [640]       & [640]          & 9.121  & [251]        &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [640]; distance of 2.0 kpc: [640]; discovered by INTEGRAL: [251]; very strong
H$\alpha$ emission with EW of $-$50\AA: [640]; lack of radio emission: [606].
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
RX J0146.9+6121 & 01 47 00.2    & LS I +61$^\circ$235 & 11.45, 0.62, $-$0.41 & 9.899 & 1--3           &        \\
                & +61 21 23.7   & V831 Cas            & B1Ve, 0.87           & 9.700 & (0.1--2.4 keV) & 1404.2 \\
                & 129.5, $-$0.8 & [278]               & [116, 634]           & 9.486 & [538]          & [266]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [602]; in open cluster NGC 663: [687]; $v_rsin i \sim$ 200 \kms: [634]; X-ray
obs.: [510]; X-ray outburst: [266]; physical parameters and V/R variability: [634]; long-term optical and IR
variability: [636]; distance of 2.3 kpc: [116].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J01583+6713 & 01 58 18.44 &       &       & 11.481 & 14           &  \\
                & 67 13 23.5  &       & Be,   & 11.033 & (20--40 keV) &  \\
T               & 129.4, 5.2  &       & [270] & 10.601 & [729]        &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [270]; hard X-ray transient, not detected in the 40-80 keV band: [729]; 7.7'
from 1RXS J015918.4+671807: [729]; USNO-B1.0 POSS II magnitudes of B=14.98, R=13.24, I=12.12; strong H$\alpha$ and weak
H$\beta$ emission lines, typical features of a Be/X-ray binary: [270]; highly absorbed, with $N_H$ approximately
10$^{23}$ cm$^{-2}$: [380].
 }\\


\noalign{\smallskip}\hline \noalign{\smallskip}
1E 0236.6+6100 & 02 40 31.7  & LS I +61$^\circ$303 & 10.7, 0.8, $-$0.3 & 8.621 & 0.2          & 26.496      \\
               & +61 13 46   & V615 Cas            & B0Ve, 0.75        & 8.228 & (0.2--5 keV) &             \\
R              & 135.7, +1.1 & [278]               & [179, 316, 726]   & 7.917 & [43]         & [755, 254] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o,r): [256]; X-ray source: [43]; two-peak accretion/ejection model: [757, 478, 496];
radio outbursts: [755, 756]; long-term radio obs.: [629]; four-year modulation radio outbursts: [184, 579, 254]; fast
precessing relativistic radio jet: [495]; microquasar ($\mu$Q): [494]; VLBI radio jet: [493, 757]; optical light curve:
[506, 578]; opt. spectra: [437, 316, 392]; orbital solution: [316, 478, 79, 254]; $v_rsin i \sim$ 113 \kms: [79];
system velocity: [795]; long-term optical obs.: [256, 438, 437]; IR obs.: [156, 311]; distance about 2.4 kpc: [217,
726]; UV obs.: [306, 315, 316, 463]; wind structure: [816]; in the error of 3EG J0241+6103: [388]; simultaneous
X-ray/radio obs.: [280]; low-mass BHC: [621]; mwl obs.: [725]; orbital period: [580, 581, 856, 492, 418, 254];
eccentricity of 0.72: [478, 79]; ejected from cluster IC 1805: [522].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
V 0332+53    & 03 34 59.9    & BQ Cam & 15.1--15.4, 1.6--2.3,  & 11.817 & $<$0.5--1250 & 34.25      \\
EXO 0331+530 & +53 10 24     &        & O8.5Ve, 1.9            & 11.206 &              & 4.4             \\
T, P, C      & 146.1, $-$2.2 & [389]  & [137, 302, 552]        & 10.744 & [730, 761]   & [547, 730, 832] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [389]; X-ray outbursts: [730, 761, 832]; X-ray obs.: [461]; rapid X-ray
variability: [35]; X-ray cyclotron line: [460]; multiple cyclotron lines: [108]; X-ray pulse phase sp.: [783]; QPO:
[747, 622]; optical spectrum: [354, 737]; $v_rsin i \sim 150$ \kms: [137]; system velocity: [795]; IR obs.: [113]; wind
structure: [816]; tilted equatorial plane: [553]; distance of 7 kpc: [553]; eccentricity of 0.37: [858, 730].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 0352+309   & 03 55 23.0     & X Per   & 6.0--6.6, 0.29, $-$0.82 & 6.149 & $<$9--37 & 250.3      \\
              & +31 02 59      &         & B0Ve, 0.4               & 6.073 &          & 835        \\
P, C          & 163.1, $-$17.1 & [65]    & [319, 451, 528, 710]    & 5.920 & [64]     & [162, 547] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; X-rays: [660]; X-ray sp.: [830]; long-term optical record: [435, 532];
disappearance emission lines: [435, 566]; system velocity: [795]; $v_rsin i \sim$ 250--400 \kms: [314, 528, 827]; UV
obs.: [40, 275]; stellar parameters: [189]; opt. polarimetry: [409]; envelope structure: [760]; photometry and
polarimetry obs. during disc loss: [666]; fundamental parameters: [451]; mwl study: [665]; cyclotron line
($B=3.3\times10^{12}$ G): [109]; orbital parameters ($e=0.11$): [162]; distance of 0.7--1.3 kpc: [189, 451, 666, 760].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J0421+560   & 04 19 42.2    & CI Cam     & 9.25--11.83, 1.0, $-$0.4 & 7.502 & 2000        & 19.41 \\
                & 55 59 59      &            & sgB[e], 0.8              & 5.741 &             &       \\
T, R            & 149.2, +4.1   & [176]      & [104, 105, 327]          & 4.323 & [37, 712]   & [28]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [394]; rapid X-ray outbursts: [221, 712]; mwl obs.: [37]; optical outbursts:
[221, 663]; B[e]: [37]; sgB[e] star: [104, 663, 327]; IR spe.: [104]; opt./IR/radio obs.: [105]; long-term UBVRIJHK
obs.: [39]; a WD: [571, 221, 346, 28]; likely a BHC: [37, 663]; distance 1--$>$5 kpc: [37, 104, 519, 346, 523, 663];
E(B$-$V) between 0.65 and 1.54: [104, 663, 571]; orbital parameters (e=0.62): [28]; B4 III--V: [28]; unusually strong
FeII lines: [176]; two-component wind: [663]; radio obs. (failed jet?): [519]; flare peaked successively from X-ray,
optical to radio: [221]; rapid changed X-ray $N_H$: [37, 589].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
RX J0440.9+4431 & 04 40 59.3    & LS V +44 17 & 10.78, 0.61, $-$0.36 & 9.500 & 1       &        \\
                & 44 31 49      & BSD 24-491  & B0.2Ve, 0.65         & 9.317 &         & 202.5  \\
P               & 159.8, -1.3   & [145]       & [539, 641]           & 9.182 & [632]   & [632]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [300]; distance 3.3 kpc: [539, 641]; optical spe.: [641]; H$\alpha$ EW
decreasing with IR magnitude fainter: [641]; $vsin i$=235 \kms: [641].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
EXO 051910+3737.7  & 05 22 35.2  & V420 Aur   & 7.51, 0.14, $-$0.86 & 6.696 & 1            &    \\
1H 0521+373        & +37 40 34   & HD 34921   & B0 IVpe, 0.42       & 6.507 &              &    \\
                   & 170.0, +0.7 & [719]      & [74, 604, 676]      & 6.230 & [215, 850]   &    \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [719]; EXO 051910+3737.7 not the same X-ray src of 1H 0521+373 in SIMBAD; hard
X-ray spectrum: [604]; UV/opt./IR obs.: [604, 676]; IR spe.: [104]; unclB[e] star: [104].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1A 0535+262  & 05 38 54.6    & V725 Tau  & 8.9--9.6, 0.45--0.62, $-$0.54 & 8.368 & $<$3--2800 & 111       \\
H 0535+262   & +26 18 57     & HD 245770 & O9.7IIIe, 0.8                 & 8.272 &            & 104       \\
T, P, C      & 181.4, $-$2.6 & [429]     & [228, 465, 726, 734]          & 8.157 & [64]       & [547, 616] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; long-term X-ray obs.: [616]; hard X-ray obs.: [115, 655, 699]; long-term
optical record: [38, 734, 452]; opt. spectr.: [3, 320, 324]; $v_rsin i \sim 300$ \kms: [320]; system velocity: [795];
mwl obs.: [164, 356]; X-ray/opt. relation: [454]; UV obs.: [164, 594, 853]; accretion model: [537]; wind structure:
[816]; disc loss \& renewal: [267]; IR spe. obs.: [103]; long-term opt./UV spe.: [102]; cyclotron lines: [260, 404];
QPO during a giant outburst: [208]; orbital elements (e=0.47): [208]; distance of 2 kpc [726] and 2.9 kpc in [452];
X-ray pulsations during disc loss phase: [558]; variable $\gamma$-ray emission: [672].
 }\\


\noalign{\smallskip} \hline \noalign{\smallskip}
1H 0556+286   & 05 55 55.1     & HD 249179  & 9.2,~~ ,   & 9.366 & 1.1      &        \\
              & +28 47 06      &            & B5ne,      & 9.238 &          &        \\
              & 181.3, +1.9    &            & [608, 778] & 9.068 & [850]    &        \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [778]; Be star: [810]; distance of 0.83 kpc: [54]; likely not an X-ray binary:
[771].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
IGR J06074+2205  & 06 07 26.6   &         &            & 10.49 & 7           &   \\
                 & 22 05 483    &         & Be,        & 10.19 & (3--10 keV) &  \\
T                &              &         & [272]      & 9.96  & [88]        &   \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [272]; discovery: [88]; $B=13.3$, $R=12.1$: [272]; opt. emission line, a
Be/X-ray binary: [272]; the radio source unrelated: [272].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
SAX J0635.2+0533 & 06 35 18.29   &         & 12.83, +0.98,     &  & 0.55       & 11.2   \\
SAX J0635+0533   & 05 33 06.3    &         & B2V--B1IIIe, 1.2  &  &            & 0.0338 \\
P                & 206.1, $-$1.0 & [363]   & [363]             &  & [363]      & [151, 364]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [363]; opt. emission line: [363]; within the error of
2EG J0635+0521: [363]; distance $\sim$ 2.5--5 kpc: [363]; eccentr. of 0.29: [364].%M=10\msun
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1WGA J0648.0$-$4419 & 06 48 04.6     & HD 49798 & 8.27, $-$0.24, $-$1.18 & 8.862 & 0.03  & 1.55      \\
RX J0648.1$-$4419   & $-$44 18 58.4  &          & sdO6,                  & 9.005 &       & 13.1789   \\
P                   & 253.7, $-$19.1 &          & [359]                  & 9.072 & [347] & [347, 762] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [598]; distance 650 pc: [347]; very soft X-ray: [347]; UV sp.: [71]; likely a
NS: [347]; a WD system(?): [45]; eccentricity of 0.03: [762].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J0658$-$073 & 06 58 17.30   & [M81] I-33  & 12.05--12.38, 1.02--0.86,  & 9.664 & 67          &         \\
MXB 0656$-$072  & $-$07 12 35.3 &             & O9.7Ve,                    & 9.332 & (2--12 keV) & 160.7   \\
T, P, C         & 220.1, $-$1.8 &             & [576]                      & 9.013 & [534]       & [534] \\
\\
\multicolumn{7}{p{17.6cm}}{ $Pos$. (o): [576]; also RX J065817.7$-$071228 and optical ctpt. GSC2 S100221212: [576];
typical of accretion-powered pulsars: [534]; hard sp. with $\alpha$=1.09: [285]; previously "soft X-ray transient":
[97]; strong cyclotron line at $\sim$35keV (B about 4$\times 10^{12}$ G): [285]; variable reddened: [576]; extremely
narrow emission lines (HI, HeI and low-ionization metals): [576].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
3A 0726$-$260 & 07 28 53.6    & V441 Pup & 11.6, 0.3, $-$0.6 & 10.366 & 1.2--4.7    & 34.5     \\
4U 0728$-$25  & $-$26 06 29   &          & O8--9Ve, 0.6      & 10.093 &             & 103.2    \\
T, P          & 240.3, $-$4.1 & [728]    & [556, 728]        & 9.832  & [815, 850]  & [138]    \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [728]; distance 4.6 or 6.1 kpc: [131, 556]; X-ray flare: [728]; opt./IR obs.:
[556]; orbital and spin periods: [138].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 0739$-$529 & 07 47 23.6     & HD 63666    & 7.62, 0.02, $-$0.24 & 7.403 & 0.7    &    \\
              & $-$53 19 57    & SAO 235515  & B7 IV--Ve,          & 7.406 &        &    \\
              & 266.3, $-$13.7 & [719]       & [456, 564, 778]     & 7.363 & [850]  &    \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [778]; parallax and proper motion: [94]; distance of 0.52 kpc: [94].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 0749$-$600  & 07 50 15.77    & HD 65663      & 6.73, 0.05, $-$0.25 & 6.542 & 0.7   &    \\
               & $-$61 05 58.2  & SAO 250018    & B8 IIIe, 0.09       & 6.571 &       &    \\
               & 272.8, $-$16.5 & [719]         & [152, 153, 778]     & 6.534 & [850] &    \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (IR): [778]; Be star: [810]; in open cluster NGC 2516: [152]; parallax and proper
motion: [94]; distance of 0.4 kpc: [94]; likely not an X-ray binary: [771].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
RX J0812.4$-$3114 & 08 12 28.4  & LS 992   & 12.48, 0.38, $-$0.29 & 11.335 & 0.6    & 81.3       \\
                  & $-$31 14 21 & V572 Pup & B0.2IVe, 0.65        & 11.126 &        & 31.8851    \\
T, P              & 249.6, +1.6 & [539]    & [637]                & 10.909 & [539]  & [133, 631] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (IR): [539]; distance about 9 kpc: [539, 637]; sharp dip in the pulse profile: [631];
Balmer lines from absorption to emission and back again to
absorption: [637]; IR mag. varied by more than 0.8 mag: [637]; $vsini=240$ \kms: [637]. %Dip, M=17\msun
}\\


\noalign{\smallskip} \hline \noalign{\smallskip}
GS 0834$-$430 & 08 35 55.4     &  $^*$D  & 20.4, ~~,          & & 30--300 & 105.8        \\
              & 43 11 11.9     &         & B0--2 III--Ve, 4.0 & &         & 12.3         \\
T, P          & 177.7, 36.7    & [349]   & [349]              & & [249]   & [249, 836] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [349]; sequence X-ray outbursts: [836]; recurrent transient: [416]; X-ray obs.:
[11]; X-ray/opt. obs.: [36]; eccentricity $0.1<e<0.17$: [836]; strong H$\alpha$ emission: [349]; spectral-type
uncertain: [349]; distance 3--5 kpc: [349]; southern of two neighboring sources: [123, 249]; IR/opt obs.: [349].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 0900$-$40 & 09 02 06.9   & HD 77581  & 6.9, 0.47, $-$0.51  & 5.833 & 2--1100 & 8.96           \\
Vela X-1     & $-$40 33 17  & GP Vel    & B0.5 Ib, 0.7        & 5.705 &         & 283            \\
P, E, C      & 263.1, +3.9  & [213]     & [182, 564]          & 5.596 & [64]    & [161, 547, 786] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; X-ray sp.: [548, 690, 830]; cyclotron line (B of 2.7$\times10^{12}$ G):
[405, 412]; pulse timing \& X-ray orbit: [62, 63, 160, 161, 627, 775, 786]; X-ray eclipses: [213, 781]; high-resolution
X-ray spectrum: [694, 241]; limits on apsidal motion: [159]; rapid X-ray variability: [35]; orbital variation X-ray
absorption: [264]; energy dependence pulse profile: [626]; opt. light curve: [766]; long-term cycles (?): [614, 766];
opt. radial-velocity curve: [793, 797]; system velocity: [795]; $v_rsin i \sim$ 90--130 \kms: [514, 766, 833]; UV obs.:
[182, 365, 502, 594, 682, 794]; high-resolution IUE obs.: [733]; opt. polarimetry: [172]; IR obs.: [238, 326]; bow
shock around the sys.: [369]; polarization: [849]; distance of 1.9 kpc [682]; runaway system from OB association Vel
OB1: [800]; 1.86$<M_x<2.27$\msun: [29, 623]; mass of GP Vel of 27.9\msun: [623]; radio emission not detected: [197].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
GRO J1008$-$57 & 10 09 46.9     & star       & 15.27, $-$1.66,  & 10.943 & 1200     & 135        \\
               & $-$58 17 35.5  &            & B0e, 1.9--2.0    & 10.272 &          & 93.5       \\
T, P           & 283.0, $-$1.8  & [117]      & [117, 657]       & 9.718  & [738]    & [706, 738] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [117]; X rays: [706]; IR and optical spectral obs.: [117]; 260 days orbital
period: [206]; e=0.66 and orbital period of 248 d: [ref. 568]; distance 5 kpc: [117]; large IR excess: [117].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
RX J1037.5$-$5647 & 10 37 35.2   & LS 1698     & 11.3, 0.9,      & & 3.3        &   \\
4U 1036$-$56      & $-$56 47 59  &             & B0V--IIIe, 0.75 & &            & 862  \\
P, T              & 285.4, +1.5  & [539]       & [539]           & & [632, 815] & [632] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 21"): [539]; X-ray flare 1974 Nov.: [815]; distance 5.0 kpc: [539]; 2 2MASS
sources in the error.
    }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1A 1118$-$615 & 11 20 57.2      & Hen 3-640     & 12.1, 0.96, $-$0.30 & 9.563 & 0.1--70    &       \\
              & $-$61 55 00     & WRAY 15-793   & O9.5Ve, 1.2         & 9.071 &            & 405   \\
P, T          & 292.5, $-$0.9   & [355]         & [355]               & 8.587 & [64, 536]  & [547] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; X-ray transient: [186, 352]; opt. phm. \& spe.: [355]; sys. velocity:
[795]; $v_rsin i \sim$ 300 \kms: [355]; X-ray/opt. obs.: [536]; opt. spe. after X-ray outburst: [605]; mwl study:
[118]; UV obs.: [112]; distance
of 5 kpc: [355].  %Po large???
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1119$-$603 & 11 21 15.1     & V779 Cen   & 13.3, 1.07, $-$0.04  & 10.736 & 10--312  & 2.09       \\
Cen X-3       & $-$60 37 25.5  &            & O6.5 II--III, 1.4    & 10.311 &          & 4.84       \\
P, E, C       & 292.1, +0.3    & [70, 408]  & [321, 408, 656]      & 10.093 & [64]     & [374, 547] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 0.6"): [328]; X-ray pulsations: [227, 775]; period decay: [187, 374]; X-ray
spectrum: [17, 445, 830, 847]; long-term X-ray history: [261, 345, 611, 617, 693]; X-ray eclipses: [692]; X-ray obs.:
[307, 544, 550]; aperiodic X-ray variability: [35]; QPO: [746]; cyclotron line at $\sim$30 keV (B of
$\sim3.5\times10^{12}$ G): [72]; opt. light curve: [766, 798]; opt. radial-velocity curve: [321, 541, 573]; mass of the
NS: [15]; $v_rsin i \sim 250$ \kms: [321]; system velocity: [795]; IR obs.: [238]; structure companion star: [101];
distance of 8--10 kpc: [321, 408]; outburst of GeV $\gamma$ ray and GeV pulsation: [804].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J11215$-$5952 & 11 21 46.81   & HD 306414  & 9.98, 0.59, $-$0.45 & 8.55 & 42           &  \\
                  & $-$59 51 47.9 &            & B1Ia, 0.78          & 8.34 & (20--60 keV) &  \\
T                 & 291.9, 1.1    &            & [387, 807]          & 8.19 & [444]        &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [561]; about 45' from Cen X-3: [444]; three brighter IR sources in the error:
[561]; distance $\sim$8 kpc: [561].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J11435$-$6109 & 11 44 10.7   &    &           & 11.486 &  10          & 52.46  \\
                  & $-$61 07 02  &    & B3e       & 11.236 & (18--45 keV) & 161.76  \\
T, P              & 294.9, 0.7   &    & [135]     & 11.107 & [252]        & [335, 744]  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [135]; $B = 13.17$: [135]; X-ray variable: [744]; $\neq$1RXS J114358.1$-$610736:
[135]; optical ctpt. USNO-B1.0 0288$-$0337948: [135].
 %???  1.3E-10  erg s-1 cm-2 at 2-10 keV: [335]
}\\


\noalign{\smallskip} \hline \noalign{\smallskip}
2S 1145$-$619  & 11 48 00.0     & V801 Cen     & 9.3, 0.18, $-$0.81 & 8.677 & 4--1000  & 187.5      \\
2E 1145.5-6155 & $-$62 12 25    & HD 102567    & B0.2IIIe, 0.35     & 8.577 &          & 292.4      \\
P, T           & 295.6, $-$0.2  & [65]         & [568, 564, 816]    & 8.403 & [64]     & [547, 819] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; X-ray spectrum: [830]; X-ray obs.: [508]; long-term X-ray history: [617,
819]; opt. spectrum: [828]; $v_rsin i \sim 270 km/s$: [275]; system velocity: [795]; coordinated X-ray/opt. obs.:
[128]; UV obs.: [42, 163, 275, 594]; wind structure: [816]; mwl obs.: [731]; optical sp. type: [see 568]; distance of
3.1 kpc
[552] and 1.4 kpc [322]. %Watson et al (1981MNRAS.195..197) suggested e =0.8
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1E 1145.1$-$6141 & 11 47 28.6     & V830 Cen   & 13.1, 1,5, 0.15 & 9.607 & 4--70       & 14.4       \\
                 & $-$61 57 14    &            & B2Iae, 1.6      & 9.110 &             & 298        \\
P                & 295.5, $-$0.01 & [322]      & [166, 331]      & 8.810 & [322, 50]   & [628, 414] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o 2"): [322]; X-ray outburst: [50]; X-ray pulsations: [828]; period of 10.76 d from
opt. sp.: [325]; system velocity: [795]; 15' away from 1145-619: [414, 829]; orbital elements ($e=0.2$ and $f(m)=5.1$
\msun): [628]; distance of 8 kpc: [331].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1223$-$624   & 12 26 37.6       & BP Cru ?   & 10.8, 1.76, 0.42    & 6.717 & 9--1000  & 41.59      \\
GX 301$-$2      & $-$62 46 13      & WRA 977    & B1--1.5 Ia, 1.8.4   & 6.077 &          & 696        \\
P, T, C         & 300.1, $-$0.04   & [65]       & [57, 274, 764, 805] & 5.672 & [64]     & [547, 689] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o 3"): [64]; X-ray spectrum: [830]; recurrent outbursts: [615, 677, 820]; X-ray
obs.: [262, 419, 423, 658, 826]; pulse-phase spectr.: [421]; pulse profile: [524]; X-ray dips: [422]; aperiodic X-ray
variability: [35, 753]; rapid spin-up episodes: [393]; optical spectrum: [274, 323, 586, 764]; optical photom.: [796];
system velocity: [795]; IR obs.: [238]; a hypergiant (?): [368]; distance of 1.8 and 5.3 kpc: [368, 586]; variable
cyclotron line (B of 3.4--5.8$\times10^{12}$G): [406, 413, 570]; eccent. 0.46: [393, 689].
%Dip
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J12349$-$6434 & 12 34 54.7    & RT Cru   & 12.46, 1.75, 0.28  & 6.646 & 1.3           &    \\
                  & $-$64 33 55.6 &          & O--A,              & 5.583 & (0.5--10 keV) &    \\
T, P              & 301.2, $-$1.8 &          & [96]               & 5.185 & [777]         &    \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 6"): [777]; discovery: [92]; optical ctpt. RT Cru?: [487]; accreting sys.: [487];
irregular variable: [96]; large-amplitude ($\triangle V=3.8$$^m$) outburst and short-term flickering: [96]; symbiotic
star: [96]; tentatively a HMXB.
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 1238$-$599  & 12 42 01.0      &           &     &     & 3--16           &             \\
3A 1239$-$599  & $-$60 12 00     &           &      &    &                 & 191         \\
P              & 301.8, +2.7     & [175]     &       &   & [64, 815, 850]  & [309]       \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 30"): [175]; hard X-ray spectrum: [309]; see also: [78].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1A 1244$-$604  & 12 47 35          &            &     &        & $<$24--100  &         \\
               & $-$60 38 34       &            &      &       &             &         \\
T              & 302.5, +2.2       &            &       &      & [78]        &         \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 6.2'): [78].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1A 1246$-$588 & 12 49 36          &        &       &       & $<$24--300    &       \\
4U 1246$-$58  & $-$59 07 18       &        &        &      &               &       \\
T             & 302.7, +3.7       &        &         &     & [78]          &       \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 4.5'): [78].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 1249$-$637 & 12 42 50.3      & HD 110432      & 5.31, 0.27, $-$0.79 & 4.655 & 2.2      &      \\
              & $-$63 03 31     & SAO 252002     & B0.5IIIe, 0.40      & 4.339 &          & 14200?  \\
              & 302.0, $-$0.2   & BZ Cru [719]   & [111, 564]          & 4.038 & [850]    & [771]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [778]; Be star: [810]; UV obs.: [111]; interstellar absorption lines: [149];
optical obs.: [155, 212]; variable radial velocity: [73]; distance of 0.3 kpc: [94]; 14 ks period: [771]; a Be/WD
candidate?: [771].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 1253$-$761 & 12 39 14.6     & HD 109857      & 6.49, 0.08, $-$0.24 & 6.169 & 0.6     &        \\
              & $-$75 22 14    & SAO 256967     & B7 Vne, 0.20        & 6.169 &         &        \\
              & 302.1, $-$12.5 & [719]          & [111, 564]          & 6.102 & [850]   &        \\
\\
\multicolumn{7}{p{17.5cm}}{ $Pos$. (o): [778]; Be star: [810]; visual double (sep. 2.2"): [202]; no optical brightness
variations: [20]; white-dwarf accretor(?): [818]; distance of 0.24 kpc: [94].
}\\


\noalign{\smallskip} \hline \noalign{\smallskip}
1H 1255$-$567 & 12 54 36.9   & $\mu^2$ Cru    & 5.17, $-$0.12, $-$0.51 & 5.316 & 0.8      &        \\
              & $-$57 10 07  & SAO 240367     & B5 Ve, 0.04            & 5.383 &          &        \\
              & 303.4, +5.7  &                & [564, 710]             & 5.313 & [850]    &        \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [778]; Be star: [810]; $v_rsin i \sim 220 km/s$: [710]; visual double with
$\mu^1$ Cru: [299]; slow \& small optical variability: [597]; distance of 0.11 kpc : [94].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1258$-$61 & 13 01 17.1    & V850 Cen    & 13.5--14.2, 1.7, 0.8 & 9.798 & 0.3--200  & 133?   \\
GX 304-1     & $-$61 36 07   & $^*$2 (MMV) & B0.7Ve, 2.0          & 9.297 &           & 272      \\
P, T?        & 304.1, +1.2   & [489]       & [136, 568, 585]      & 9.040 & [64, 601] & [547, 617] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (IR): [489]; long-term X rays: [614, 617]; X-ray off state: [601]; X-ray spectrum:
[658, 830]; opt. spectrum: [489, 764]; sp.-type B2V: [552]; long-term opt. variations: [136]; $v_rsin i \sim 600$ \kms:
[585]; system velocity:
[795]; IR obs.: [238]; distance of 2.4 kpc: [585].  %e large in [568]
}\\

 \noalign{\smallskip}\hline \noalign{\smallskip}
2RXP               & 13 01 58.7    &    &         & 13.0 & 6.3          &       \\
J130159.6$-$635806 & $-$63 58 09   &    &         & 12.1 & (20--60 keV) & 704   \\
T, P               & 304.1, $-$1.1 &    & [93]    & 11.4 & [93]         & [93]  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (IR): [93]; quick spin-up: [93]; distance 4--7 kpc: [93]; hard X-ray spectrum: [93];
a high mass X-ray binary with Be companion: [93].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
SAX J1324.4$-$6200 & 13 24 26.3   &          &     & & 0.4      &        \\
                   & $-$62 00 53  &          &     & &          & 170.84 \\
P                  & 306.8, +0.61 &          &     & & [9]      & [9] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 1.5'): [9]; distance $>$3.4 kpc: [9]; hard X-ray sp.:
[9]; likely a Be/X-ray system: [9]. %???Po=27 h, LMXB: [Lin et al. 02]
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
2S 1417$-$624 & 14 21 12.9       & $^*$7    & 17.2:, 0.7:1.7, 0.8  & 13.297 & 2--43    & 42.12     \\
              & $-$62 41 54      &          & B1Ve, 2:             & 12.747 &          & 17.6     \\
P, T          & 313.0, $-$1.6    & [13]     & [258]                & 12.294 & [64]     & [207, 373] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; X-ray obs.: [13, 207, 373]; opt. id: [258]; orbital parameters (e= 0.45):
[207]; Centaurus 1971--2 transient (?): [123]; 1994 II-type outburst: [207]; X-ray outburst: [333]; distance of
1.4--11.1 kpc: [258].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
SAX J1452.8$-$5949 & 14 52 49.3     &               &            & & 0.04       &       \\
                   & $-$59 49 18    &               &            & &            & 437.4 \\
P                  & 317.6, $-$0.44 &               &            & & [569]      & [569] \\

\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 50"): [569]; X-ray sp.: [569]; distance 6--12 kpc: [569]; probably a Be/X-ray
binary: [569].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1538$-$52 & 15 42 23.3  & QV Nor     & 14.4, 1.9, 0.6  & 10.358 & $<$3--30 & 3.73        \\
             & $-$52 23 10 & $^*$12     & B0 Iab, 2.1     & 9.910  &          & 529         \\
P, E, C      & 327.4, +2.2 & [12]       & [147, 330, 584] & 9.677  & [64]     & [31, 158]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; distance of 4.5 to 6.4 kpc: [100, 648]; X-ray obs.: [122, 459, 661]; X-ray
eclipses: [31, 158]; X-ray orbit: [459]; X-ray spectrum: [459, 830]; X-ray cyclotron line at $\sim$21 keV : [98, 662];
long-term spin-up trend: [679, 662]; eccentricity of 0.174: [99]; orbital decay $-$2.9$\times10^{-6}$ yr$^{-1}$: [99];
opt. light curve: [575]; radial-velocity curve: [147, 648]; $v_rsin i \sim 200 km/s$: [147]; system velocity: [795];
opt. obs.: [584].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
XTE J1543$-$568 & 15 44 01      &  &  &  & 8       & 75.56      \\
                & $-$56 45.9    &  &  &  &         & 27.12      \\
T, P            & 325.0, $-$1.5 &  &  &  & [475]   & [342, 475] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 2'): [342]; a BeXRB at $d\geq10$ kpc: [342]; orbital parameters (e$<$0.03 and
f(M)=8.2\msun): [342].
%e is the lowest for the 12 Be/x-ray binaries whose orbits have now been measured)
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
2S 1553$-$542 & 15 57 49.0       &            &       &     & 27        & 30.6       \\
              & $-$54 24 54      &            &       &     &           & 9.3        \\
P             & 327.9, $-$0.9    & [12]       &       &     & [64]      & [375, 547] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 3.5"): [64]; opt. counterpart likely a Be star: [375]; X-ray orbit: [375];
e$<$0.09: [375].
}\\


\noalign{\smallskip} \hline \noalign{\smallskip}
1H 1555$-$552 & 15 54 21.8    & HD 141926      & 8.60, 0.56, $-$0.43 & 7.098 & 1.7       &      \\
              & $-$55 19 45   & SAO 243098     & B2IIIn,             & 6.841 &           &      \\
              & 327.0, $-$1.2 & [719]          & [192, 806]          & 6.509 & [850]     &      \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [778]; Be star: [810]; distance of 0.96 kpc: [257]; Herbig Ae/Be star?: [806];
low luminosity BeXRB: [771].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16195$-$4945 & 16 19 29   & HD 146628? & 10.08, 0.44,    & 8.575 & 9        &  \\
AX J1619.4$-$4945 & $-$49 45.5 &            & B1--2Ia,        & 8.412 &          &  \\
                  & 333.5, 0.3 & [707]      & [707]           & 8.377 & [707]    &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 1'): [707]; optical ctpt HD 146628?: [707]; variable, highly absorbed hard
spectrum: [707]; likely a neutron star in a HMXB: [707]; distance of 7
kpc: [707]. %???in a high state with flux of $\sim$17 mCrab at 20-40 keV: [707].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16283$-$4838 & 16 28 10.7  &         &    & 16.798 & 13           &   \\
                  & $-$48 38 55 &         &    & 15.815 & (20--40 keV) &   \\
                  & 335.3, 0.10 & [33]    &    & 13.948 & [33]         &   \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 5"): [33]; highly absorbed (variable) and flat X-ray spectrum: [33]; possible IR
counterpart in the 2MASS and Spitzer survey: [33]; a HMXB containing a NS: [33].
%30.7 mJy =
}\\

 \noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16318$-$4848 & 16 31 48.31   & $^*$ 1 & $>$21.1,~~ , & 10.33   & 45      &   \\
                  & $-$48 49 00.7 &        & ~~, 5.6           & $<$10.4 &         &   \\
                  & 335.6, $-$0.4 & [205]  & [205]             & $<$9.1  & [498]   &   \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [205]; the first source discovered by INTEGRAL: [143, 813]; very high absorption
($N_H>10^{24}$ cm$^{-2}$): [813, 205, 498]; very strong Fe K$\alpha$ emission line and significant K$\beta$ and Ni
K$\alpha$ lines: [498]; IR ctpt.: [216]; previous ASCA outburst in 1994: [543]; I=16.05, R=17.72: [205]; a HMXB with a
B0--B5 sgB[e] at a distance between 0.9--6.2 kpc: [205].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16320$-$4751  & 16 32 01.9    & $^*$ 1  &    & 14.080 & 17      & 8.96    \\
AX J1631.9$-$4752  & $-$47 52 27.1 &         &    & 13.028 &         & 1309   \\
P                  & 336.3, 0.17   & [671]   &    & 10.986 & [343]   & [142, 450] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 4"): [671]; discovery: [767]; heavily absorbed: [669, 343]; persistent for at
least 8 years: [343]; star '1' IR ctpt: [671]; SG/X-ray binary?: [343].
%the fourth source from a new class of highly absorbed binary systems for which the pulsations are observed.
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16358$-$4726 & 16 35 58       &   &  &  & 7        &   \\
                  & $-$47 24.4     &   &  &  &          & 5880  \\
T, P              & 337.1, $-$0.00 &   &  &  & [591]    & [591]  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 2'): [44]; no radio emission detected; heavily absorbed source: [44]; probably a
HMXB with spin 5880 s: [591]; Fe K$\alpha$ emission line: [591]; rough distance of $\sim$6--8 kpc: [645].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
AX J1639.0$-$4642  & 16 39 05.4   &  &    & 14.633 & 0.8          &         \\
IGR J16393$-$4643  & $-$46 42 14  &  &    & 13.316 & (0.7--10keV) & 912.0   \\
P                  & 338.01, 0.07 &  &    & 12,780 & [51]         & [51] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (IR): [51]; IR ctpt 2MASS J16390535$-$4642137; huge $N_H$, hard spectral index,
probably a HMXB: [742, 120, 51]; well within the error of 3EG J1639$-$4702: [120]; large variations in intensity: [51];
X-ray lines: [51]; the radio ctpt [120] out of the XMM error: [51].
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16418$-$4532 & 16 41 45    &  &  &  & 1            &  \\
                  & $-$45 31 12 &  &  &  & (20--40 keV) &   \\
                  & 339.2, 0.5  &  &  &  & [446]        &   \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 2'): [768]; in the Norma Region: [768]; heavily absorbed $N_H \sim 10^{23}
cm^{-2}$: [410]; a HMXB?: [410].
}\\


\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16465$-$4507 & 16 46 35.26   &  &           & 10.537 & 16           &  \\
                  & $-$45 07 04.5 &  & B0.5I,    & 10.079 & (18--60 keV) & 228 \\
T, P              & 340.1, 0.13   &  & [560]     & 9.843  & [446]        & [447] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (IR): [560]; $B=15.2$, $R=13.0$: [714]; fast X-ray transient: [446]; extremely
absorbed ($N_H\sim 7\times 10^{23} cm^{-2}$): [447]; very high rotational velocity: [560]; 2MASS source (J=10.54) and
No. 0448-0520455 in the USNO B1.0 catalog; distance of 12.5 kpc: [714].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16479$-$4514 & 16 48 07.0     &  & $\sim$20.4, ~~ ,   & 12.954 & 470          &  \\
                  & $-$45 12 05.8  &  &                    & 10.825 & (20--30 keV) &  \\
T                 & 304.2, $-$0.12 &  & [379]              & 9.798  & [704]        &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 6"): [379]; fast transient: [704]; a faint source with V$\sim$20.4: [379];
$N_H=1.2\times10^{23}cm^{-2}$: [447]; IR source IRAS 16441$-$4506 in the error: [704]; outburst or type I burst?:
[704]; a NS in a HMXB?: [447, 704].
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J16493$-$4348 & 16 49 21     &  &  &  & 0.4    &  \\
                  & $-$43 48 36  &  &  &  &        &  \\
                  & 341.4, 0.6   &  &  &  & [472]  &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 2'): [253]; in the Norma Region: [253]; only 45" off the radio pulsar PSR
J1649$-$4349: [253]; variable on time scales of 100 to 1000 s: [472]; no significant pulsations: [472]; heavily
absorbed power law ($N_H \sim 10^{23} cm^{-2}$ and $\alpha$=1.4): [472]; a HMXB?: [410].
}\\

%\noalign{\smallskip}\hline \noalign{\smallskip}
%IGR J16558-5203  & 16 56 05.6   &  & B=14.5, R=13.5 &   &  \\
%                 & -52 03 40.4  &  &                &   &  \\
%                 &              &  & [0G7]          &  &  \\
%\\
%\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [0G7]; in the Norma region; associated with a bright
%ROSAT src: [0G7]; possible extended?: [0G7] = Stephen, J.B. 2005, A\&A, 432, L49
%}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
OAO 1657$-$415 & 17 00 48.9    & star     &                          & 14.665 & 4--42 & 10.4       \\
               & $-$41 39 21.6 &          & B SG, 6.6                & 13.778 &       & 38         \\
P, E           & 344.4, 0.31   & [83]     & [83]                     & 13.383 & [64]  & [81, 547] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 0.5"): [83]; V861 Sco not the optical ctpt.: [14]; X-ray obs.: [366]; X-ray
spectrum: [830]; hard X-ray obs.: [509]; X-ray eclipsing: [81]; orbital solution: [81]; highly reddened: [83]; distance
of 6.4 kpc: [83]; iron K emission line: [83].
} \\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1700$-$37 & 17 03 56.8  & HD 153919 & 6.6, 0.27, $-$0.72  & 5.744 & $<$11--110 & 3.41  \\
             & $-$37 50 39 & V884 Sco  & O6.5Iaf$^+$, 0.52   & 5.639 &            &       \\
E, C         & 347.8, +2.2 & [362]     & [276, 596, 848]     & 5.496 & [64]       & [362] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [64]; eclipsing system: [362]; X ray during strong flares and eclipse: [789];
X-ray variab.: [35, 174, 265]; hard X-ray sp.: [600]; no X-ray pulsations: [174, 246]; X-ray sp. lines: [789, 58];
QPO?: [58]; broad cyclotron absorption feature at $\sim$37 keV?: [649]; opt. light curve: [19, 799]; opt. sp.: [125,
154, 191, 287]; radial-velocity curve: [174, 273, 277]; $e=0.22$: [277]; $v_rsin i \sim$ 140--300 \kms: [125, 154, 313,
848]; system velocity: [795]; UV obs.: [181, 276, 367]; soft X-ray Raman scattering: [367]; opt. polarimetry: [171,
172]; polarization: [849]; IR obs.: [238, 596]; system parameters: [281]; possibly 13.81 days period: [395, 303];
runaway from OB association SCO OB1: [10]; decrease in orbital period: [265]; physical parameters with
$\dot{M}=9.5\times10^{-6}$ \msun/yr, M$_* = 58$\msun and M$_x = 2.44$\msun: [106]; low mass BHC?: [649]; distance of
1.9 kpc: [10].
 } \\

\noalign{\smallskip} \hline \noalign{\smallskip}
AX J1700$-$419     & 17 00 5.3     &       &      &     & 0.4      &        \\
AX J170006$-$4157  & $-$41 57 44   &       &      &     &          & 714.5  \\
P                  & 344.0, +0.25  &       &      &     & [770]    & [770] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 1'): [770]; a WD binary also possible: [770].
}\\

 \noalign{\smallskip}\hline \noalign{\smallskip}
IGR J17091$-$3624  & 17 09 02.3    &  &  & & 22           &  \\
                   & $-$36 23 33   &  &  & & (15--40 keV) &  \\
T, R               & 349.5, 2.2    &  &  & & [411]        &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (r): [680]; radio ctpt: [680]; radio obs., microquasar?: [577]; X-ray large
variability: [448, 411]; BHC: [448]; uncertain if a Be/X-ray binary or LMXB: [343].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
EXO 1722$-$363    & 17 25 11.4       &         &        & 14.218 & 0.2--8      & 9.74        \\
IGR J17252$-$3616 & $-$36 16 57.5    &         &        & 11.811 &             & 413.9       \\
P, E              & 351.5, $-$0.35   &         &        & 10.672 & [754, 141]  & [141, 754] \\
\\
\multicolumn{7}{p{17.5cm}}{ $Pos$. (IR): [861]; 2MASS J17251139-3616575: [861]; apparent total eclipses: [141]; hard
X-ray spectrum: [754]; very large $N_H$: [749, 861]; Fe K$\alpha$ line at 6.4 keV: [861]; at Galactic bulge region:
[749]; mass function: [141]; a SG/X-ray binary: [141,
861].  %Zurita Heras, J.A. et al. 2005, A\&A, astro-ph/0511115
%0-15 mCrab at 2-10 keV: [141];
 }\\


\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J1739$-$302   & 17 39 11.58    &             & 14.89, 2.97, 1.68  & 8.600 & 136         &       \\
IGR J17391$-$3021 & $-$30 20 37.6  &             & O8Iab(f), 3.4      & 7.823 & (2--25 keV) & 1500?   \\
T                 & 358.1, 0.45    &             & [562]              & 7.428 & [715]       & [684]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x): [718]; fast transient: [715, 718]; USNO A2.0 (0525 28760590) and 2MASS source:
[718]; highly reddened: [562]; radio obs.: [295]; radio source 2' away from the Chandra source: [681]; X-ray spec:
[715]; distance of $\sim$2.3 kpc: [562].
}\\

 \noalign{\smallskip} \hline \noalign{\smallskip}
RX J1739.4$-$2942 & 17 39 30.1    &    &      &   & 2.5         &  \\
GRS 1736$-$297    & $-$29 42 07   &    &      &   & (3--12 keV) &  \\
T                 & 358.6, $-$0.7 &    &      &   & [593]       &    \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 19.2"): [540]; hard X-ray spec.: [540]; X-ray observation: [593, 842]; a Be/X-ray
binary instead of LMXB?: [540]; LMXB in SIMBAD.
}\\

 \noalign{\smallskip}\hline \noalign{\smallskip}
AX J1740.1$-$2847 & 17 40 11.6   &  &  &  & 0.2     &        \\
                  & $-$28 47 48  &  &  &  &         & 729    \\
P                 & 359.5, 1.1   &  &  &  & [683]   & [683] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 30"): [683]; possibly a HMXB near the Galactic center region: [683].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
RX J1744.7$-$2713 & 17 44 45.7  & V3892 Sgr   & 8.4, 0.44, $-$0.64 & 7.054 & 0.06   & \\
                  & $-$27 13 44 & HD 161103   & B0.5V--IIIe,       & 6.843 &        & \\
                  & 1.36, +1.1  &             & [180, 727]         & 6.507 & [539]  &  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [727]; strong emission lines: [539]; distance 0.8 kpc: [539]; IR photom. and
spectrum: [724, 308]; $vsini =224$ \kms: [727].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
AX J1749.1$-$2733 & 17 49 06    &              &        &      & 0.2           &    \\
                  & $-$27 33    &              &        &      & (0.7--10 keV) &     \\
T                 & 1.58, 0.06  &              &        &      & [684]         &    \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x ?): [684]; fast X-ray transient: [684, see also 334]; HMXB?: [560].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
AX J1749.2$-$2725 & 17 49 10.1  &              &        &      & 1.36         &        \\
                  & $-$27 25 16 &              &        &      &              & 220.38    \\
T, P              & 1.7, +0.1   &              &        &      & [769]        & [769]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 1'): [769]; weak X-ray source: [769]; hard X-ray sp.: [769, 684]; likely a BeXRB
with NS: [769]; within error of a nearby WD: [769]; distance 8.5 kpc: [769].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
GRO J1750$-$27 & 17 49 12.7   &                &           &      & 56       & 29.8 \\
               & $-$26 38 36  &                &           &      &          & 4.45  \\
P, T           & 2.4, +0.5    &                &           &      & [698]    & [698] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 4"): [698]; no optical counterpart reported: [698]; likely Be system: [698]; large
spin-up: [698]; orbital parameters (e=0.36): [698]; distant
source (18 kpc?): [698]. %100mCrab (20-50 keV)
  }\\

 \noalign{\smallskip}\hline \noalign{\smallskip}
IGR J17544$-$2619       & 17 54 25.28   & * C1    & 12.65, 1.79,  & 8.791 & 89          &  \\
1RXS J175428.3$-$262035 & $-$26 19 52.6 &         & O9Ib, 2.07    & 8.310 & (17--45keV) &  \\
T                       & 3.2, $-$0.34  & [595]   & [595]         & 8.018 & [250]       &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (IR 0.2"): [668]; short X-ray flare: [743, 250]; 2MASS J17542527-2619526 and also in
the USNO B1.0 Catalogue: [668]; ultra-soft quiescent X-ray: [334]; a NS: [334]; distance of 8 kpc or between 3--4 kpc:
[243, 595].
%[743]Sunyaev, R. A. et al. 2003, ATel 190 [250]Grebenev, S. A. et al. 2003 ATel 192
%????160 mCrab, in the 18-25 keV bands: [ooo]
}\\

 \noalign{\smallskip}\hline \noalign{\smallskip}
SAX J1802.7$-$2017 & 18 02 39.9    &  &  &  & 1.5           & 4.6      \\
IGR J18027$-$2016  & $-$20 17 13.5 &  &  &  & (0.1--10 keV) & 139.61   \\
T, P, E            & 9.4, 1.04     &  &  &  & [18]          & [18]   \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 2'): [18]; $\sim22'$ away from the bright X-ray source GX 9+1: [18]; system
parameters ($e\leq$0.2 and $f(M)\sim17\pm5\msun$): [18, 291]; an eclipsing HMXB (at distance of 10 kpc?): [18, 291].
}\\


\noalign{\smallskip}  \hline \noalign{\smallskip}
4U 1807$-$10   & 18 11         &            &         &     & $<$2--10   &   \\
               & $-$10 54      &            &         &     &            &   \\
T              & 18.6, +3.9    &            &         &     & [215]      &   \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 1.3$^\circ$): (large error box): [215]; uncertain if HMXB or LMXB.
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
SAX J1818.6$-$1703 & 18 18 39      & HD 168078? & 10.7, $-$0.1,  & & 56         &  \\
                   & $-$17 03 06   &            & B3III,         & & (2--9 keV) &  \\
T                  & 14.1, $-$0.73 &            & [338]          & & [338]      &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 3'): [338]; fast transient: [704]; optical ctpt HD 168078?: [338].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
SAX J1819.3$-$2525 & 18 19 21.48   & V4641 Sgr   & 8.8--13.5, $-$0.2, 1.8 & 12.532 & 1--13000    & 2.8    \\
XTE J1819$-$254    & $-$25 25 36.0 &             & B9III, 0.32            & 12.364 & (2--12 keV) &        \\
T, R               & 6.8, $-$4.8   & [244]       & [572, 741]             & 12.27  & [713]       & [572] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o 0.7"): [686]; misidentified as GM Sgr: [686]; X-ray light curve: [339]; strong
relativistic Fe-K$\alpha$ emission line: [339, 515]; X-ray flare sp.: [339, 457]; fast and large X-ray outbursts: [713,
834]; X-ray sp. harder during decay and considerably softer in quiescent state: [834]; opt. outburst: [741, 87]; opt.
sp.: [572]; radio obs., highly relativistic jet ($\mu$Q): [298]; orbital period: [370, 572]; mass of the compact star
9.6 M$_{\odot}$: [572]; distance between 7--12 kpc: [87, 572]; super-Eddington outburst: [646].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
AX J1820.5$-$1434 & 18 20 29.5    &         &             &  & 8         &         \\
                  & $-$14 34 24   &         & O9.5--B0Ve  &  &           & 152.26  \\
P                 & 16.5, +0.07   &         & [350]       &  & [449]     & [382]   \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 0.5'): [382]; X rays: [449]; $R = 17.33$: [350]; a highly obscured accreting
binary: [382]; distance of 4.7 kpc: [382].
% detection of hard X-ray emission at $\sim$10--15 mCrab in the 15--40 energy band: [449]; 3.3e-11.
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
RX J1826.2$-$1450 & 18 26 15.06     & LS 5039    & 11.23, 0.94, $-$0.16 & 9.024 & 0.3   & 3.90   \\
                  & $-$14 50 54.3   &            & ON6.5V((f)), 1.28    & 8.751 &       &       \\
R                 & 16.9, $-$1.3    & [539]      & [504, 539]           & 8.604 & [539] & [80] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (r): [653]; distance 2.5 kpc: [80]; small optical photom. var.: [482]; radio ctpt.:
[479]; X-ray and radio obs.: [651, 652]; X-ray variability: [60, 638]; relativistic jet, $\gamma$-ray-emitting
persistent ($\mu$Q): [582, 583]; orbital X-Ray variability: [60]; low X-ray state: [484]; optical polarimetry: [121];
orbital parameters: [504, 80]; $e=0.35$ and $M_X=3.7$ (a BHC?): [80]; runaway: [653, 503]; very high energy $\gamma$
rays: [5].
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
XTE J1829$-$098 & 18 29 44.0   &   &    &  & 4       &        \\
                & $-$09 51 23  &   &    &  &         & 7.82   \\
T, P            & 21.7, 0.28   &   &    &  & [471]   & [471] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 4"): [268]; $I=14.4$: [269]; heavily absorbed ($N_H \sim$ $10^{23} cm^{-2}$):
[471]; hard spectrum favoring a HMXB: [471]; 8" away from a very bright SG star in 2MASS (with J=8.04, H=6.11, K=4.98):
[269].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
H 1833$-$076 & 18 36 28.6     &             &      &    & 1.6--200         &            \\
Sct X-1      & $-$07 36 21    &             &      &    &                  & 111        \\
P, T         & 24.5, $-$0.16  & [247]       &      &    & [399, 618, 815]  & [403, 547] \\
\\
\multicolumn{7}{p{17.5cm}}{ $Pos$. (x 30"): [630]; alternative position: [630]; X-ray obs.: [86, 292]; X-ray
pulsations: [403]; hard X-ray spectrum: [129, 630]; long-term X-ray record: [618]; transient: [129].
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
AX J1838.0$-$0655  & 18 38 01      &  &  &  & 0.5          &  \\
                   & $-$06 55 54   &  &  &  & (0.7--10keV) &  \\
                   & 25.2, $-$0.19 &  &  &  & [742]        &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 1.0'): [742]; $N_H=1.1\times10^{23}cm^{-2}$, probably a HMXB: [742]; a SNR or a
pulsar with nebula: [462]; high-energy cutoff value above 30 keV (BHC?): [447].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
GS 1839$-$04   & 18 41 48     &            &      &    & 2.5          &       \\
               & $-$04 27     &            &      &    &              & 81.1  \\
P, T           & 27.9, +0.11  &            &      &    & [399]        & [399] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 24'): [399].
 }\\


\noalign{\smallskip} \hline \noalign{\smallskip}
GS 1839$-$06  & 18 41 42     &       &     &     & 1        &   \\
              & $-$05 51     &       &     &     &          &   \\
T             & 26.6, $-$0.5 &       &     &     & [399]    &   \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 30'): [399].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
AX J1841.0$-$0536  & 18 41 00.43    &   &     & 9.74 & 4       &  \\
IGR J18410$-$0535  & $-$05 35 46.5  &   &     & 9.22 &         & 4.7394   \\
T, P               & 26.8, $-$0.24  &   &     & 8.93 & [22]    & [22] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (o): [271]; fast transient: [22]; $B=15.91$, $R=12.78$: [271]; distance 10 kpc?: [22,
271]; 6.4 keV line: [22]; heavily absorbed hard spectrum: [22, 271]; weak H$\alpha$ emission: [271].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
GS 1843+009   & 18 45 36.8    & star       & 20.2,                  &  & 33        &       \\
              & 00 51 48.3    &            & B0--B2IV--Ve, 2.3--2.9 &  &           & 29.5  \\
P, T, C       & 33.0, 1.7     & [351]      & [351]                  &  & [399]     & [399] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [351]; X-ray obs.: [399, 400, 603]; hard X-ray outburst: [845, 89]; possible
cyclotron feature (B = 1.7$\times10^{12}$G): [512]; V$-$R = 2.1: [351]; distance $\geq$10 kpc: [351]; strong H$\alpha$
emission: [351].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
2S 1845$-$024  & 18 48 18     &           &     &      & 1--44        & 241        \\
GS 1843$-$02   & $-$02 25 12  &           &     &      &              & 94.8       \\
P, T           & 30.4, $-$0.4 & [247]     &     &      & [64, 399]    & [859, 399] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 30"): [64]; also known as 4U 1850-03 and GRO J1849-03; X-ray obs.: [177, 399, 401,
700]; distance: of 10 kpc: [399]; likely a Be/X-ray: [720, 209]; X-ray outburst: [209]; high eccentricity (0.88):
[209].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
AX 1845.0$-$0433  & 18 45 02      &         & 13.96, 2.2, 1.04 & & 45            &    \\
IGR J18450$-$0435 & $-$04 33 31   &         & O9.5I, 2.45      & & (0.7--10 keV) &    \\
T                 & 28.8, $-$1.22 & [119]   & [119]            & & [854]         &    \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 1'): [119]; fast transient: [854]; discovery of x-ray source: [854]; optical
spectrum: [119]; distance 3.6 kpc: [119].
}\\

\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J18483$-$0311  & 18 48.3     &  & &  & 22           &  \\
                 & $-$03 11      &  & &  & (15--40 keV) &  \\
T                & 29.8, $-$0.7  &  & &  & [91]         &  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 2'): [91]; in the Scutum arm, probably a HMXB: [343].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
GS 1855$-$02   & 18 58       &           &       &     & 2         &    \\
             & $-$02 44      &           &       &     &           &    \\
T            & 31.2, $-$2.7  & [132]     &       &     & [399]     &   \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 10'): [399].
  }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J1855$-$026  & 18 55 31.3  &           &        &    & 6         & 6.067  \\
               & $-$02 36 24   &           &        &    &           & 361    \\
P, T, E        & 31.1, $-$2.1  & [132]     &        &    & [139]     & [139]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 12"): [132]; iron emission line: [139]; most likely a SG/X-ray system: [139, 132];
BD-2 4786 not the opt. cpt.: [139]; X-ray sp.: [139]; within the error of src No. 6 in [399]: [139]; an extended
near-total eclipse system: [132]; orbital parameter (e$<$0.04): [132]; consistent with a B0I star: [132]; highly
absorbed: [132]; an early-type star (B=16.1, I=11.5) right on the edge of the ASCA error: [803]; distance $\sim$ 10
kpc: [139].
  }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J1858+034  & 18 58 36      & star?     & 18.0, 1.6, &  & 25       &       \\
               & 03 26 09      &           &            &  &          & 221.0 \\
P, T           & 36.8, $-$0.02 & [640]     & [640]      &  & [643]    & [748] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [640]; 0.11 Hz QPO: [592]; outburst: [529]; very hard X-ray sp.: [592, 643];
probably a Be/X-ray sys.: [748]; emission-line optical ctpt. though out of the JEM-X error: [640].
}\\


\noalign{\smallskip}\hline \noalign{\smallskip}
XTE J1859+083  & 18 59.1   &   &  &  & 8       &       \\
               & 08 15     &   &  &  &         & 9.801 \\
T, P           & 41.1, 2.1 &   &  &  & [474]   & [474] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 2'): [474]; X-ray pulsar: [474]; tentatively a HMXB.
% \bibitem[]{}[474] Marshall, F. E. et al. 1999, IAUC, 7240
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J1901+014         & 19 01 39.90    & star   & 18.72, 2.44, & & 500         &   \\
1RXS J190141.0+012618 & 01 26 39.2     &        &              & & (2--12 keV) &   \\
T                     & 35.4, $-$1.6   & [612]  & [612]        & & [644]       &   \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [612]; fast transient: [644].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1901+03  & 19 03 37.1    &        &       &  & $<$2--333  & 22.58  \\
            & +03 11 31     &        &       &  &            & 2.763  \\
P, T        & 37.2, $-$1.25 & [224]  &       &  & [123, 224] & [224] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (x 1'): [224]; transient 1971: [123, 214]; hard X-ray spectrum: [123]; distance of 10
kpc?: [224]; the longest (32.2 yr) recurrence X-ray transient: [224]; orbital parameters (e = 0.036 and
F$_x$(M)=2.58\msun): [224]; lack of bright IR ctpt.: [224]; unlikely SG companion: [224]; accreting from the wind of OB
main-sequence star?: [224].
%8e-9 (= 240 mCrab) at 2.5 -25 keV: [224].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J1906+09  & 19 04 47.48   & star   &  & 15.18 & 0.3--5   &       \\
              & 09 02 41.8    &        &  & 14.17 &          & 89.17 \\
P, T          & 42.5, 1.2     & [240]  &  & 13.50 & [839]    & [473] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [240];  R=18.7: [240]; distance $\geq10$ kpc: [473]; likely a Be/X-ray binary:
[473, 839, 240]; X-ray outbursts: [473, 839, 240]; orbital period between 26--30 d: [839]; low eccentricity
(0.03--0.06): [839].
%Lx=1.1e-10 at 2-10keV: [839?????] 7E36
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1907+09   & 19 09 39.3      & star        & 16.4, 3.2,     & & 4--275    & 8.38       \\
H 1907+097   & +09 49 45       &             & O8--9 Ia, 3.45 & &           & 438        \\
P, T, C      & 43.7, +0.5      & [696]       & [144, 696]     & & [64]      & [458, 477] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [696]; distance $\sim$5 kpc: [144]; long-term X-ray record: [618]; 1980
outburst: [477]; cyclotron lines at $\sim$19 and $\sim$39 keV (B of 2.1$\times10^{12}$ G); [150]; heavily reddened
massive star with broad H$\alpha$ emission: [696]; orbital parameters: [127, 458]; orbital modulation X-ray flux:
[477]; X-ray dip due to cessations of the mass accretion rather than occultation: [336]; long-term spin-down: [337]; e
= 0.28: [337]; opt. spectrum: [353, 791]; $v_rsin i \sim$ 85 \kms: [791].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
3A 1909+048  & 19 11 49.6      & SS 433         & 14.2, 2.1, 0.6  & 9.398 & 2--10       & 13.1   \\
             & +04 58 58       & V1343 Aql      & pec, 2.6        & 8.739 &             &        \\
E, R         & 39.7, $-$2.2    & [425]          & [466, 546, 811] & 8.163 & [64]        & [146]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o,r): [64]; X-ray obs.: [23, 35, 68, 69, 259, 372]; Doppler shift X-ray Fe line:
[497, 822]; extended X-ray lobes: [701, 821]; $\gamma$-ray obs.: [226, 415]; Doppler shifted opt. emission lines: [464,
467]; high-speed jet velocity (v$\sim$0.26) ($\mu$Q): [4, 235]; stationary emission lines from accretion disk: [204];
kinematic model with precessing of 164 d: [4, 183]; opt. spe.: [190, 193, 397, 468]; opt. spectrophot.: [6, 396, 811];
opt. lt. curve: [16, 288, 424, 426, 427]; long-term optical phot.: [288, 377, 499]; X-ray/opt. eclipse: [732]; IR obs.:
[390, 814]; precession clock: [7]; radio structure: [24, 195, 196, 673, 722, 801]; radio variability: [56, 203];
distance 4.61 in [736], 5.5 kpc in [296, 49]; nature of the compact star: [170]; circularly polarized radio emission:
[199]; BH with a mid-A SG sys.: [293, 90]; evolutionary status: [381]; absorption features from accretion disc wind?:
[25]; sharp variations in the X-ray, IR and radio, double X-ray Fe line profiles from the jet: [85]; massive ejection
event with a QPO-like feature near 0.1 Hz: [398]; extended radio emission: [48]; X-ray dominated by precessing jets:
[551, 476]; bullet-like jets: [84]; highly ionized Doppler-shifted iron emission lines: [511]; identifiable deviations
from the traditional kinematic model: [49]; rapid chaotic optical variability: [647].
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
4U 1909+07 & 19 10 48.2    & $^*$ A  &               & 13.228 & 1--7   & 4.4        \\
X1908+075  & +07 35 52.3   &         & OI7.5--9.5    & 11.457 &        & 604.68     \\
P          & 41.9, $-$0.81 & [533]   & [533]         & 10.480 & [824]  & [824, 428]  \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (IR): [533]; distance 7 kpc: [533]; highly-absorbed: [824]; orbital inclination angle
(38$^\circ$--72$^\circ$): [428]; e=0.021, f(M)=6.07\msun: [428].
}\\


\noalign{\smallskip}\hline \noalign{\smallskip}
IGR J19140+0951   & 19 14 04.2    &       &         & 8.55 & 75--100     & 13.558 \\
IGR J19140+098    & 9 52 58.3     &       &         & 7.67 & (1--20 keV) &        \\
                  & 44.3, $-$0.46 & [344] & [344]   & 7.06 & [670]       & [140] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x 0.6"): [344]; also known as EXO 1912+097: [443]; a HMXB with a NS: [670]; variable
absorption column density: [670]; bright iron line: [670]; IR ctpt. 2MASS 19140422+0952577: [344].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 1936+541    & 19 32 52.3     & DM +53$^\circ$2262  & 9.8, ~~,   & 10.231 & 0.7     &      \\
               & +53 52 45      &                     & Be,        & 10.166 &         &      \\
               & 85.9, +15.9    &                     & [778]      & 9.975  & [850]   &      \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [778]; Be star: [810]; X-ray emission not detected: [771]; consistent with a
quiescent Be/NS sys.: [771].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
XTE J1946+274  & 19 45 39.3  & $^*$A    & 16.9, 1.72,           & 12.539 & $<$ 1--25   & 169.2      \\
GRO J1944+26   & 27 21 55.4  &          & B0--1 IV-Ve, 1.9--2.2 & 11.831 & (2--60 keV) & 15.8       \\
P, T, C        & 63.2, +1.4  & [802]    & [802]                 & 11.333 & [745]       & [841, 711] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [802]; transient Nov-Dec 1976: [815]; X-ray flare: [76]; $\sim$80 day period:
[76]; very hard X-ray spec.: [711]; distance of 9.5 kpc: [802, 841]; $e=0.33$ and $f(M)=9.7$\msun: [841]; IR excess and
strong H$\alpha$ emission: [802]; cyclotron line at 36.2 keV ($B=4.2\times10^{12}$ G): [283].
              %,110mcrab(2-60 keV)=7 e-9 = 25????: [745]
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
KS 1947+300    & 19 49 30.5     & $^*$3  & 14.24, 0.93, $-$0.09 & 11.67 & $<$ 10--375 & 40.4    \\
GRO J1948+32   & +30 12 24      &        & B0Ve, 1.09           & 11.43 &             & 18.7    \\
P, T           & 66.1, +2.1     & [248]  & [559]                & 11.21 & [59]        & [82, 223]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [248]; H$\alpha$ emission: [245, 559]; IR photom. (J=11.67, H=11.43, K=11.21):
[559]; distance about 10 kpc: [559]; eccentricity 0.033: [223]; mass function: [82]; frequency glitch: [223].
% 9e-9 (2-60keV): [223]
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 1956+35  & 19 58 21.7    & HD 226868    & 8.9, 0.84, $-$0.26 & 6.872 & 235--1320  & 5.     \\
 Cyg X-1    & +35 12 06     & V1357 Cyg    & O9.7 Iab, 1.06     & 6.652 &            &        \\
U, R        & 71.3, +3.1    & [624]        & [124, 157, 564]    & 6.501 & [64]       & [231]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o,r): [64]; hard X- and $\gamma$- ray obs.: [230, 432, 685, 697, 779, 780];
long-term X-ray obs.: [301, 620, 239, 610, 857, 835]; X-ray low/high states: [431, 751]; X-ray dips: [21, 384, 642];
rapid X-ray variability: [34, 35, 442, 505, 525, 526, 527, 678]; QPO: [219, 808]; chaotic (?): [441, 785]; 300 d
period: [232, 376, 378, 620]; X-ray spectrum: [26, 27, 188, 385, 445, 809]; $\gamma$-ray obs.: [433, 599]; radio obs.:
[66, 67, 294, 297]; opt. spectra: [1, 124, 233, 234, 565]; radial-velocity curve: [231, 232, 565]; $v_rsin i \sim 100$
\kms: [233]; system velocity: [795]; nature of the compact star: [52, 705, 823]; opt. light curve: [378, 453]; opt. UV
polarimetry: [173, 218, 849]; UV obs.: [157, 181, 774, 852]; IR obs.: [420]; fund. parameters, $M_*=17.5$\msun and
$M_x=10.1$\msun: [290]; massive BH formed without SN: [521]; dark jet: [222]; precession of the inner accretion disk:
[773]; model constraint on the masses: [860]; focused companion wind: [517]; quenched millimeter emission: [765]; short
cutoff timescales: [201]; distance about 2.14 kpc: [491]; broad-band X-ray spectra: [329]; giant outburst: [242];
powerful millisecond flares: [229]; radio jets with a speed in excess of 0.6c ($\mu$Q): [735]; orbital elements: [236];
probing the inner region: [168]; X-ray/optical sp.: [752]; composite Fe K$\alpha$ emission line: [516];
short-time-scale correlations between line and continuum fluxes: [455]; soft Gamma-ray spectral variability: [501];
high-resolution X-ray spectrum: [695]; temporal evolution of X-ray lags: [609]; very
flat radio-millimetre spectrum: [200]; X-ray sp.: [237]; orbital modulation: [607].%Dip
 }\\

\noalign{\smallskip}\hline \noalign{\smallskip}
W63 X-1            & 20 19     &   &  &  & 1.5            &        \\
2E 2017.1+4553 ?   & +45 42    &   &  &  & (0.3--4.5 keV) & 36     \\
P                  & 82.3, 5.4 &   &  &  & [703]          & [650] \\
\\
\multicolumn{7}{p{17.6cm}}{$Pos$. (x ?): [846]; in the northern part of SNR W63 [846] (G82.2+5.3), possibly associated
with the SNR: [650]; distance between 1.3--1.9 kpc: [674]; much harder than diffuse soft X-ray emission from SNR W63:
[650]; possible counterpart having H$\alpha$ excess emission: [650]; HMXB with a Be companion: [650].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
EXO 2030+375   & 20 32 15.2   & $^*$2       & 19.7, 3.3,  & 12.05  & $<$0.5--1400 & 46.02        \\
               & +37 38 15    & V2246 Cyg   & B0Ve, 3.8   & 10.835 &              & 41.8          \\
P, T           & 77.2, $-$1.3 & [114, 535]  & [114, 535]  & 10.074 & [587]        & [547, 587, 739] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o 2"): [535]; giant outburst: [587]; rapid X-ray variability: [35]; 0.2 Hz QPO: [8];
opt. spe.: [114, 357]; long-term opt./IR variability: [635]; distance of 7.1 kpc: [840]; eccentricity of 0.41: [840];
X-ray outburst at apastron: [417]; transition from global spin-down to spin-up: [843].
}\\


\noalign{\smallskip} \hline \noalign{\smallskip}
4U 2030+40  & 20 32 26.5       & V1521 Cyg      &               & 15.309 & 90--430     & 0.20     \\
Cyg X-3     & +40 57 09        &                & WR star, 6.3  & 13.192 &             &          \\
R           & 79.8, +0.7       & [812]          & [792]         & 11.921 & [64]        & [590]    \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (r): [64]; I=20.0: [812]; distance about 10 kpc: [167]; orb. period change: [386,
787, 709]; long-term X-ray obs.: [301, 619]; no X-ray pulsations: [386, 851]; orbital X-ray curve: [54, 383]; aperiodic
variability: [35, 61]; X-ray halo: [530]; transient QPO: [788]; radio outbursts: [255, 360, 567]; quiescent radio
flares (period 4.95 h?): [531]; two-sided relativistic jet ($\mu$Q): [481, 480, 740]; one-sided highly relativistic
jet: [225, 520]; IR phot.: [32, 488, 490]; IR spectra: [371, 792]; X-ray spectrum: [383, 825]; sp. variability during
outburst and quiescence: [198]; VLBI obs. during outburst: [691]; intense stellar wind: [613, 790]; correlated behavior
between hard X-ray and radio: [500]; hot spots excited by jets: [483]; hard X-ray time lag: [95]; multifrequency radio
observations: [518]; extended X-ray emission: [284]; $\gamma$-ray obs.: [563]; Doppler shifts of the X-ray emission
lines: [723]; high-resolution X-ray spectroscopy: [574].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
RX J2030.5+4751  & 20 30 30.8     & SAO 49725       & 9.27, 0.38, $-$0.65 & 8.058 & 0.04      &  \\
                 & 47 51 51       & BD +47 3129     & B0.5V--IIIe,        & 7.854 &           &   \\
                 & 85.2, +5.0     & [539]           & [539]               & 7.624 & [539]     &  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [300]; strong emission lines: [539]; distance 2.2 kpc: [539]; likely Be/X-ray
binary: [539].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
GRO J2058+42          & 20 58 47.5  & star    & 14.92, 1.12,        & 11.74  & 320         & 55.03  \\
CXOU J205847.5+414637 & 41 46 37    &         & O9.5--B0IV--Ve, 1.4 & 11.282 &             & 198   \\
P, T                  & 83.6, 2.7   & [844]   & [640]               & 10.930 & [837]       & [837, 844]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [640]; giant outburst in 1995: [837]; distance 9.0 kpc: [640]; Chandra obs.:
[844]; optical ctpt to the Chandra src 3" outside the GRO error: [844]; strong H$\alpha$ emission line: [844]; 2MASS
source: [844]; pulsations not detected with Chandra: [844].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
SAX J2103.5+4545 & 21 03 35.7    & star        & 14.2, 1.12, & 11.842 & 20            & 12.68     \\
                 & 45 45 04      &             & B0Ve, 1.36  & 11.535 &               & 358.61 \\
P, T             & 87.12, $-$0.7 & [639]       & [639]       & 11.362 & [30]          & [30, 310]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [639]; HD200709 not opt. cpt.: [30]; X-ray spe.: [310]; large spin-up: [708];
0.044Hz QPO: [332]; eccentricity 0.4$\pm$0.2: [30]; distance of 6.5 kpc: [639]; fast optical spectral variability:
[639]; $v sini=240$\kms: [639].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 2138+579  & 21 39 30.6    & V490 Cep  & 14.29, ~~ ,   & 11.829 & $<$6--100  &           \\
Cep X-4      & +56 59 12.9   &           & B1--B2Ve, 1.3 & 11.414 &            & 66.2       \\
P, T, C      & 99.0, 3.3     & [53]      & [53, 53]      & 10.926 & [402]      & [402, 547] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [667]; X-ray obs.: [402]; X-ray cyclotron line (B=2.5$\times10^{12}$ G): [513];
same as Cep X-4(?): [470, 782]; X-ray outburst: [838]; orbital period 23--147.3 days: [838]; distance of 3.8 kpc: [53];
$v sini$ 460 \kms: [53].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
1H 2202+501    & 22 01 38.2      & BD +49$^\circ$3718  & 8.8, 0.17,  & 8.778 & 0.7         &          \\
               & +50 10 05       & V2175 Cyg           & Be, 0.30    & 8.701 &             &          \\
               & 97.2, $-$4.0    & [719]               & [778]       & 8.496 & [850]       &          \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [778]; Be star: [810]; distance of 0.7 kpc: [94].
}\\

\noalign{\smallskip} \hline \noalign{\smallskip}
4U 2206+543   & 22 07 56.2     & BD +53 2790 & 9.85, 0.2, $-$0.6 & 9.218 & 0.6--5.5    & 9.57        \\
3A 2206+543   & +54 31 06      &             & O9.5Ve, 0.5       & 9.116 &             &             \\
C             & 100.6, $-$1.1  & [728]       & [728, 555]        & 9.038 & [815, 850]  & [134, 654]  \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o): [300]; X rays: [688]; NS system: [772, 485, 46, 654]; Be/WD system: [134];
distance 2.6 kpc: [47]; 392 s pulsation? [688] not true: [134]; cyclotron resonant feature at 32 keV
(B=3.6$\times10^{12}$ G): [772, 485, 46]; not typical Be, but peculiar O9.5V star with relatively strong wind: [46,
555]; very low wind terminal velocity of $\sim$350 \kms: [654]; moderate eccentricity around 0.15?: [654]; wind-fed
HMXB with ms donor: [654].
 }\\

\noalign{\smallskip} \hline \noalign{\smallskip}
SAX J2239.3+6116 & 22 39 20.90   & star      & 15.1, 1.4,      & 11.450 & 16      & 262        \\
1H 2214+589      & +61 16 26.8   &           & B0V-B2IIIe, 1.4 & 10.955 &         & 1247       \\
T, P             & 107.7, +2.3   & [340]     & [340]           & 10.557 & [340]   & [340, 341] \\
\\
\multicolumn{7}{p{17.5cm}}{$Pos$. (o 0.3"): [340]; distance of 4.4 kpc: [340]; position coincided with 4U 2238+60 and
3A 2237+608: [340].
}\\

\noalign{\smallskip} \hline
\end{tabular}
\end{table*}


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