/ftp/cats/J_other/PZ/16.213



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J/other/PZ/16.213   Variable stars in the globular cluster M92  (Kheilo, 1967)
The following files can be converted to FITS (extension .fit or fit.gz)
	stars.dat measures.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/other/PZ/16.213
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drwxr-xr-x 13 cats archive 246 Jun 27 2016 [Up] drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 482 Dec 19 2022 .message -r--r--r-- 1 cats archive 4879 May 31 2013 ReadMe -rw-r--r-- 1 cats archive 241 Feb 13 2013 +footg5.gif -rw-r--r-- 1 cats archive 2071 Feb 13 2013 +footg8.gif -r--r--r-- 1 cats archive 25598 Feb 11 2013 measures.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 640 Jan 21 2013 stars.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/other/PZ/16.213 Variable stars in the globular cluster M92 (Kheilo, 1967) ================================================================================ Variable Stars in Globular Cluster M92 Kheilo E.S. <Perem. Zvezdy, 16.213 (1967)> =1967PZ.....16..213K ================================================================================ ADC_Keywords: Stars, variable Keywords: Abstract: 10 RR Lyr-type variables in M92 are studied. Data obtained from observations carried out by the author (1961-1965) and those of the past years were used. Periods of brightness variations, diagrams O-C, mean curves, period-amplitude and period-asymmetry relations were determined. Variations of the periods of studied variables were discovered; 3 of them do not possess Blazko effect. A distance of 10.5kpc to M92 was obtained according to the media,n magnitude of the studied stars.