Grids of Stellar Models - Part Three - from 0.8 to 120-SOLAR-MASSES at Z=0.004

Details Grids of Stellar Models - Part Three - from 0.8 to 120-SOLAR-MASSES at Z=0.004 Grids of Stellar Models - Part Three - from 0.8 to 120-SOLAR-MASSES at Z=0.004

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as..101..415c&link_type=abstract

Astronomy and Astrophysics Supplement, Vol.101, NO.2/OCTII, P. 415, 1993

Astronomy and Astrophysics

Astrophysics

226

Stars: Evolution Of, Stars: Hertzsprung-Russel Diagram

Scientific paper

Stellar evolutionary models with mass loss and moderate overshooting at metallicity Z = 0.004 in the 0.80 to 120 Msun range are presented. They complete the set of grids computed with the same up- input physics for Z = 0.020 and 0.001 by Schaller et al. (1992), for Z = 0.008 by Schaerer et al. (1992) and for Z = 0.040 by Schaerer et al. (1993).

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