========================================================================== J/A+A/337/403 Low-mass stars evolutionary models (Baraffe+ 1998) The following files can be converted to FITS (extension .fit .fgz or .fiZ) tab1-3.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+A/337/403 ==========================================================================
drwxr-xr-x 7 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:58 [TAR file] -rw-r--r-- 1 cats archive 459 Sep 27 1998 .message -r--r--r-- 1 cats archive 3378 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 36906 Jul 31 1998 tab1-3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/337/403 Low-mass stars evolutionary models (Baraffe+ 1998) ================================================================================ Evolutionary models for solar metallicity low-mass stars: mass-magnitude relationships and color-magnitude diagrams Baraffe I., Chabrier G., Allard F., Hauschildt P. <Astron. Astrophys. 337, 403 (1998)> =1998A&A...337..403B (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Stars, masses ; Models, evolutionary ; Photometry Keywords: stars: low-mass, brown dwarfs - stars: evolution - stars: Hertzprung-Russel (HR) and C-M diagrams - stars: interiors - stars: atmospheres Description: Physical properties and absolute magnitudes of low-mass stars for different initial metallicity [M/H], helium mass fraction Y and mixing length parameter Lmix: mass (in solar mass), age (in Gyrs) effective temperature (in K), log of gravity (in cgs) and absolute magnitudes. The VRI magnitudes are in the Johnson-Cousins system and the JHK magnitudes in the CIT system. Note that the bolometric magnitude corresponds to M_bol(Sun)=4.64. The lowest mass corresponds to the hydrogen-burning limit.
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