========================================================================== J/A+AS/110/553 Teff for B, A and F main sequence stars (Sokolov, 1995) The following files can be converted to FITS (extension .fit .fit.Z .fgz) table3 ========================================================================== Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+AS/110/553 ==========================================================================
drwxr-xr-x 21 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jun 16 11:01 [TAR file] -rw-r--r-- 1 cats archive 459 Dec 9 1997 .message -rw-r--r-- 1 cats archive 2372 Oct 28 1997 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 11750 Jan 6 1995 table3
Beginning of ReadMe : J/A+AS/110/553 Teff for B, A and F main sequence stars (Sokolov, 1995) ================================================================================ The determination of Teff of B, A and F main sequence stars from the continuum between 3200 A and 3600 A. SOKOLOV N.A. <Astron. Astrophys. Suppl. Ser. 110, 553 (1995)> =1995A&AS..110..553S (SIMBAD/NED Reference) ================================================================================ ADC_Keywords: Spectrophotometry; Ultraviolet; Stars, B-type; Stars, A-type; Stars, F-type; Effective temperatures Keywords: stars: atmospheres - stars: early-type - stars: fundamental parameters Description: A method of determination of the effective temperature of B, A and F main sequence stars is proposed, using the slope of the continuum between 3200A and 3600A. We have determined the Balmer jump and the effective temperatures for 235 main sequence stars.
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