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II/195B ==OBSOLETE version of Catalogue==
20-Sep-1999: See Last Version of GCVS = II/214
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/195B
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-r--r--r-- 1 cats archive 20690 Sep 26 1997 id73.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
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-r--r--r-- 1 cats archive 18438 Sep 26 1997 nl73.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
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Beginning of ReadMe :II/195B Namelists of variable stars Nos.67-73 (Khopolov+, 1985-97)
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The computer-readable namelists of Variable Stars Nos.67-73
Kholopov P.N., Samus N.N., Kazarovets E.V., Perova N.B.
<IAU Inform. Bull. Var. Stars, 2681, 1 (1985)>
Kholopov P.N., Samus N.N., Kazarovets E.V., Kireeva N.N.
<IAU Inform. Bull. Var. Stars, 3058, 1 (1987)>
Kholopov P.N., Samus N.N., Kazarovets B.V., Frolov M.S., Kireeva N.N.
<IAU Inform. Bull. Var. Stars, 3323, 1 (1989)>
Kazarovets E.V., Samus N.N.
<IAU Inform. Bull. Var. Stars, 3530, 1 (1990)>
Kazarovets E.V., Samus N.N., Goranskij V.P.
<IAU Inform. Bull. Var. Stars, 3840, 1 (1993)>
Kazarovets E.V., Samus N.N.
<IAU Inform. Bull. Var. Stars, 4140, 1 (1995)>
Kazarovets E.V., Samus N.N.
<IAU Inform. Bull. Var. Stars, 4471, 1 (1997)>
=1985IBVS.2681....1K
=1987IBVS.3058....1K
=1989IBVS.3323....1K
=1990IBVS.3530....1K
=1993IBVS.3840....1K
=1995IBVS.4140....1K
=1997IBVS.4471....1K
================================================================================
ADC_Keywords: Stars, variable
Authors' addresses:
Description:
We present a computer-readable version of six Name-Lists of Variable
Stars (Nos.67-72) published in the system introduced during the
preparation of the 4th GCVS edition. For printed versions of these
Name-Lists see IBVS No.2681,1985; No.3058,1987; No.3323,1989;
No.3530,1990; No.3840,1993; No.4140,1995. The main body of the 4th
GCVS edition is already available in computer-readable form (see
II/139, II/172, II/205).
There are 2735 stars in the Name-Lists Nos.67-72 (file "nl.dat"). The
variables are arranged in the order of their names inside
constellations. One star of the 67th Name-List (V1810 Cyg=No.67247)
turned out to be non-existing, it has been excluded from the table.
The identification table (file "ident.dat") and the list of references
(file "ref.dat") follow. The total number of designated variable stars
has now reached 31193. In the new computer-readable version 1.1 of the
GCVS, vol. IV (catalog II/172), we now present identifications
also for name-list stars.
We make no special attempt to present the material in a completely
homogeneous form. There happened minor style evolution from the 67th
to the 70th Name-List: particularly, the 67th Name-List normally
refers in the identification table only to the catalogues cited in the
papers mentioned in the references in the files "nl.dat" and
"ident.dat", and to the 70th Name-List it became a common practice to
give more catalogue identifications. From the Name-List No.70, there
is no completeness in identifications with the old catalogues of
suspected variables (CSV), in many cases we consider the NSV
identification sufficient. We also do not try to update the
information of the older Name-Lists, we only put the information
together and correct known mistakes.
The corrections to the Name-Lists have been taken into account. It is
necessary to reproduce here two remarks from forewords of the printed
Name-Lists:
Name-List No.69. In the case of the variable stars in the open cluster
NGC 3766 (V843-V849 Cen), there is some ambiguity in their
identification with the HD,CoD,CPD catalogues. In particular, we do
not agree with the HD catalogue identification of HD 100856 with
CPD-60 3102 and consider V843 Cen=CPD-60 3102 to be identical with HDE
306794; HD 100856=CPD-60 3112.
Name-List No.70. The 70th Name-List contains a number of variables in
Taurus discovered by J. Kelemen [70113]. Unfortunately the discovery
announcement contains some mistakes in co-ordinates and in
identifications with other lists. These mistakes have been corrected
according to [70114].
(Added in version II/195B)
The name-list number 73 was added at CDS on 26-Sep-1997. It was kept
in a different file because it is differently formatted (better
accuracy in the position). The references of this 73rd name list were
however merged with the previous ones in the file ref.dat.