========================================================================== J/A+A/429/309 HR 1099 radial velocities (Frasca+, 2004) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat table2.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/429/309 ==========================================================================
drwxr-xr-x 15 cats archive 4096 Feb 15 12:41 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:58 [TAR file] -rw-r--r-- 1 cats archive 480 Mar 5 2005 .message -r--r--r-- 1 cats archive 3663 Mar 5 2005 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 6360 Sep 7 2004 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 6481 Sep 7 2004 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 17541 Sep 9 2004 tables.ps.gz [Uncompressed] -r--r--r-- 1 cats archive 22192 Sep 7 2004 tables.tex
Beginning of ReadMe : J/A+A/429/309 HR 1099 radial velocities (Frasca+, 2005) ================================================================================ Orbital period variation in close binaries from radial velocity data and magnetic activity cycles. II. HR 1099. Frasca A., Lanza A.F. <Astron. Astrophys. 429, 309 (2005)> =2005A&A...429..309F ================================================================================ ADC_Keywords: Stars, variable ; Radial velocities Keywords: stars: binaries: close - stars: activity - stars: binaries spectroscopic - stars: individual: HR 1099 Abstract: We studied orbital period changes in the non-eclipsing close binary HR 1099, one of the most bright members of the RS CVn class of magnetically active binary systems. Intermediate-resolution optical spectroscopy and IUE archive spectra were used to build radial-velocity curves yielding epochs of superior conjunction with an accuracy of 0.01 days. The final database ranged from 1976 to 2002 and allowed us a better assessment of the amplitude of the orbital period variation and its timescale. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 03 36 47.3 +00 35 16 HR 1099 = HD 22468 ----------------------------------------------------------
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