/ftp/cats/VI/113



==========================================================================
VI/113     Evolutionary models of Population II stars    (Cariulo+, 2004)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	trkfiles.dat hbfiles.dat strfiles.dat isofiles.dat tracks.dat hb.dat
	isochron.dat blueloop.dat struct.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VI/113
==========================================================================

drwxr-xr-x 141 cats archive 4096 Sep 6 2023 [Up] drwxr-xr-x 4 cats archive 4096 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 553 Dec 19 2022 .message -r--r--r-- 1 cats archive 12178 Oct 3 2004 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 1492072 Oct 2 2004 hb.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -rw-r--r-- 1 cats archive 7553 Oct 3 2004 hbfiles.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 10778874 Oct 2 2004 isochron.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 35553 Sep 24 2004 isofiles.dat [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 9 cats archive 155 Oct 2 2004 models -r--r--r-- 1 cats archive 2340 Sep 25 2004 strfiles.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3400977 Oct 2 2004 struct.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 26251859 Oct 2 2004 tracks.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1300 Sep 24 2004 trkfiles.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : VI/113 Evolutionary models of Population II stars (Cariulo+, 2004) ================================================================================ Stellar evolutionary models of Population II stars. Cariulo P., Castellani V., Degl'Innocenti S. <Astron. Astrophys. 421, 1121 (2004)> =2004A&A...421.1121C ================================================================================ ADC_Keywords: Models, evolutionary ; Stars, population II Keywords: stars: evolution - globular clusters: general - open clusters and associations: general Description: The models are calculated for different chemical compositions both without overshooting (standard models, including microscopic diffusion of He and heavy elements) and with different overshooting efficiency. Each set of models can be found in a different sub-directory. It is possible to get all the content for each chemical composition, the content of each selected sub-directory or just a given file. In each directory there are evolutionary tracks (TRACKS), isochrones (ISOCHRONES), horizontal branch models together with a table of the ZAHB characteristics (HB) and files with some relevant physical values of selected models (STRUCTURES). Models with overshooting are calculated for masses higher than 1M_sun_ to avoid the unobserved presence of the overall contraction feature in 1M_sun_ stars. Thus isochrones for ages higher than about 5Gyr are the same as in the standard case and thus are not included in the overshooting directories. Models with overshooting does not include microscopic diffusion because for masses higher than about 1M_sun_ the effect of this mechanism is almost negligible. Models with overshooting are calculated for masses higher than 1M_sun_ to avoid the unobserved presence of the overall contraction feature in 1M_sun_ stars. Thus isochrones for ages higher than about 5Gyr are the same as in the standard case and thus are not included in the overshooting directories. Models with overshooting does not include microscopic diffusion because for masses higher than about 1M_sun_ the effect of this mechanism is almost negligible. All the tracks and isochrones have been transformed in the observation plane by adopting the model atmospheres by Castelli (1999A&A...346..564C), see also Castelli, Gratton & Kurucz (1997A&A...318..841C). For convenience, all tracks and isochrones have been grouped in 4 tables tracks.dat, struct.dat, hb.dat and isochron.dat