/ftp/cats/II/194A



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II/194A     Photometric study of IC 4665  (McCarthy+ 1969)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
	table1 table2
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=II/194A
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 2 cats archive 231 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 445 Dec 19 2022 .message -r--r--r-- 1 cats archive 5350 Jun 13 1995 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1920 Jun 2 1994 table1 -r--r--r-- 1 cats archive 10790 Jun 13 1995 table2
Beginning of ReadMe : II/194A Photometric study of IC 4665 (McCarthy+ 1969) ================================================================================ A photometric study of the open cluster IC 4665 McCARTHY M.F.S.J., O'SULLIVAN S.S.J. <Ricerche Astron., 7, 483-498 (1969)> =1969RA......7..483M (SIMBAD/NED RefCode) ================================================================================ ADC_Keywords: Clusters, open ; Photographic catalog Summary: Photographic observations of the open cluster IC 4665 made on blue and yellow sensitive plates with the Vatican 40 cm refractor are presented and discussed. Apparent magnitudes were determined for 200 stars by means of a program of photometric reduction designed by BERTIAU. The mean internal errors in the final blue and yellow magnitudes average about 0.02 mag. All stars selected for measurement of proper motions by VASILEVSKIS on long base-line Allegheny plates have been observed here. The forty stars which VASILEVSKIS' proper motion measures have shown to be probable members constitute a normal main sequence from V = 7 to V = 13.5, followed by a gap of 0.2 to 0.3 mag, and a group of 10 stars in the subgiant domain. The reality of this gap and the membership characteristics of the stars in the subgiant region of the C - M diagram are discussed.