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VI/118 Stellar Models until He burning (Claret+ 1995-1998)
(Merging of the 4 published papers in A&AS)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
grid.dat models.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VI/118
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Beginning of ReadMe :VI/118 Stellar Models until He burning (Claret+ 1995-1998)
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Stellar Models until He burning, Papers 1-4
Claret A., Gimenez A.
<Astron. Astrophys. Suppl. Ser. 109, 441 (1995);
Astron. Astrophys. Suppl. Ser. 114, 549 (1995);
Astron. Astrophys. Suppl. Ser. 125, 439 (1997);
Astron. Astrophys. Suppl. Ser. 133, 123 (1998)>
=1995A&AS..109..441C
=1995A&AS..114..549C
=1997A&AS..125..439C
=1998A&AS..133..123C
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ADC_Keywords: Models, evolutionary
Keywords: stars: binaries: general - evolution - interiors -
fundamental parameters - abundance
Description:
Grids of stellar evolutionary models published in the 4 papers
referenced below are merged here. OPAL opacities with LS coupling and
Grevesse composition were adopted, and Alexander's tables were used
for lower temperatures. The models adopt a core overshooting with
alpha_ov_=0.20, and mixing length parameter l/H_p_=1.52 that seems
to represent well double-lined eclipsing binary stars. Mass loss
during the main sequence and in the red giant phase were taken into
account. The nuclear network treats 14 isotopes and optionally the
lithium burning to study its depletion in less massive models during
pre main sequence evolution.
The initial parameters of the models are summarized in the file
"grids.dat", with metal contents of Z=0.02 (solar), 0.01, 0.03 and
0.004 (Magellanic Clouds), with a wide range of initial hydrogen
content around the solar composition. The mass range covered goes
from 1 (0.6 for the solar composition) up to 40M_sun_ and the more
massive models were followed until helium burning.