========================================================================== J/A+A/337/779 V810 Cen Geneva photometry (Kienzle+ 1998) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+A/337/779 ==========================================================================
drwxr-xr-x 7 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jun 16 11:03 [TAR file] -rw-r--r-- 1 cats archive 451 Sep 27 1998 .message -r--r--r-- 1 cats archive 3046 Sep 27 1998 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 37522 Jun 23 1998 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/337/779 V810 Cen Geneva photometry (Kienzle+ 1998) ================================================================================ The pulsating yellow supergiant V810 Centauri Kienzle F., Burki G., Burnet M., Meynet G. <Astron. Astrophys. 337, 779 (1998)> =1998A&A...337..779K (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Stars, supergiant ; Photometry, Geneva Keywords: stars: individual : V810 Centauri - stars: supergiants - stars: oscillations - stars: evolution - open clusters and associations: individual: Stock 14 Description: The light curve of the yellow supergiant V810 Centauri in the Geneva photometric system has been analysed with Date Compensate Fourier Transform and Weighted Wavelet Z-transform. Two periods around 150 and 100 days dominate the frequency spectrum but variable amplitudes and other modes are required to fully reproduce whole data set. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 11 43 31.2 -62 29 21 V810 Cen = HD 101947 ----------------------------------------------------------
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