/ftp/cats/J_A+AS/135/29



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J/A+AS/135/29       New periods of variable stars in Cygnus        (Hric+ 1999)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table2.dat table3.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+AS/135/29
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drwxr-xr-x 22 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 09:36 [TAR file] -rw-r--r-- 1 cats archive 479 Mar 6 2013 .message -r--r--r-- 1 cats archive 5284 Feb 11 1999 ReadMe -rw-r--r-- 1 cats archive 244 Mar 6 2013 +footg5.gif -rw-r--r-- 1 cats archive 2079 Mar 6 2013 +footg8.gif -r--r--r-- 1 cats archive 17589 Dec 7 1998 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1020 Dec 7 1998 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+AS/135/29 New periods of variable stars in Cygnus (Hric+ 1999) ================================================================================ New periods of variable stars in Cygnus based on a quarter of century of photographic observations. Hric L., Galis R. <Astron. Astrophys. Suppl. Ser. 135, 29 (1999)> =1999A&AS..135...29H (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Stars, variable ; Magnitudes Keywords: star: techniques: photometric - stars: variables: general Description: The Table2 summarizes the photographic magnitudes obtained over 24 years at the Skalnate Pleso (1979-1993) and Asiago (1969-1988) observatories for 17 variable stars of different types: Miras (7), Semi-regular (4), Cepheids (3), RR Lyr (2), Eclipsing binary (1). The cross-reference between star No., designation according to Margoni and Stagni (1984A&AS...56...87M) and catalogue one (provided it has already been adopted for a given star) according to the GCVS (See Cat. II/214) and IBVS (Kholopov al., 1987, See Cat. II/195) is given in Table3 as well as the equatorial coordinates for the epoch 1950.0 for each star, which is compatible with the GCVS. In this table are shown the basic characteristics of the observational material for each star: the number of data points and interval of magnitudes obtained at the Asiago Observatory (A) and Skalnate Pleso Observatory (SP) respectively.

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