==========================================================================
V/27 Proper Motions and UBV Photometry in h+chi Per (Muminov 1980)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
data1.dat data2.dat adjarea.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=V/27
==========================================================================
drwxr-xr-x 146 cats archive 4096 Aug 1 2023 [Up]
drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 480 Dec 19 2022 .message
-r--r--r-- 1 cats archive 6147 Apr 1 2005 ReadMe
-rw-r--r-- 1 cats archive 1012 Nov 17 2022 +footg5.gif
-rw-r--r-- 1 cats archive 3011 Nov 17 2022 +footg8.gif
-r--r--r-- 1 cats archive 62818 Oct 12 2000 adjarea.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 159350 Oct 12 2000 data1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 54779 Oct 12 2000 data2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :V/27 Proper Motions and UBV Photometry in h+chi Per (Muminov 1980)
================================================================================
Proper Motions and UBV Photometry of Stars in the Region of the
h and chi Persei Clusters
Muminov M.
<Circ. Astron. Inst. Acad. Sci. SSR, Tashkent, 98 (1982);
Bull. Inf. CDS 24, 95 (1983)>
=1983BICDS..24...95M
================================================================================
ADC_Keywords: Clusters, open ; Proper motions ; Photometry, UBV ;
Associations, stellar ; Regional catalog
Description:
Proper motions with an 80 year baseline have been determined relative
to reference stars with B=13.9mag. determined for 3086 stars brighter
than B=15.5mag. within an area of 50' radius, centered at RA=2h16.9m,
Dec=+57deg01' (1950.0). Two pairs of Tashkent normal astrograph
plates with a mean epoch difference of 80 years was used. Proper
motions were also measured for 1055 stars with 15.5 <= B <= 17.1 mag.
in two areas 14' in radius, centered on the h and chi Persei
clusters. Proper motions are also given for 1386 stars in an adjacent
area (RA=2h06.7m, Dec=+56deg57') for 1386 stars with a 38 year
baseline.
The mean errors of the proper motions are equal in right ascension and
declination. For the h and chi Perseus region, they are 0.0021"/yr
and for the adjacent region, they are 0.0031"/yr. The proper motions
in the adjacent area have been reduced to the system of those in the
cluster region using 214 stars in common.
UBV magnitudes of the stars were determined using plates taken with
the 80/120/240 Schmidt telescope of the Radioastrophysical Observatory
of the Academy of Sciences of the Latvian SSR and photoelectric
standards published by Johnson and Morgan (1955ApJ...122..429J) and
Widley (1964ApJS....8..439W). The number of measured plates and the
corresponding errors are given in the following table:
-----------------------------------------------------
FILE NAME # PLATES ERRORS (0.01mag)
V B U V B U
-----------------------------------------------------
data1.dat 2 3 2 6 5 6
data2.dat 1 2 - 8 6 -
adjarea.dat 2 2 2 6 6 6
_____________________________________________________
Cluster members were selected on the basis of their proper motion and
photometric criteria. The membership probability was calculated on the
assumption of a normal distribution of the proper motions around the
cluster proper motion.
Objects:
--------------------------------------------------------------
RA (2000) DE Designation(s)
--------------------------------------------------------------
02 19 00 +57 09.0 NGC 869 = C 0215+569 = h Per
02 22 24 +57 07.0 NGC 884 = C 0218+568 = chi Per
--------------------------------------------------------------