Grids of Stellar Models - Part Four - from 0.8-SOLAR-MASS to 120-SOLAR-MASSES at Z=0.040

Details Grids of Stellar Models - Part Four - from 0.8-SOLAR-MASS to 120-SOLAR-MASSES at Z=0.040 Grids of Stellar Models - Part Four - from 0.8-SOLAR-MASS to 120-SOLAR-MASSES at Z=0.040

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as..102..339s&link_type=abstract

Astronomy and Astrophysics Supplement, Vol.102, NO. 2/DECI, P. 339, 1993

Astronomy and Astrophysics

Astrophysics

238

Stars: Evolution, Stars: Hertzsprung-Russell (Hr) Diagram

Scientific paper

The present grid of evolutionary sequences at metallicity Z = 0.040, completes the set of grids computed for Z = 0.020 and 0.001 by Schaller et al. (1992), Z = 0.008 by Schaerer et al. (1992) and Z = 0.004 by Charbonnel et al. (1993). The models with mass loss and moderate core overshooting have been computed for 0.8 to 120 Msun using up-to-date input physics and the new radiative opacities from Iglesias et al. (1992) and Kurucz (1991).

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