Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...84..139m&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 84, no. 1, July 1990, p. 139-177.
Astronomy and Astrophysics
Astrophysics
296
Metallicity, Stellar Evolution, Stellar Mass, Tables (Data), Abundance, Astronomical Models, O Stars, Supergiant Stars, Wolf-Rayet Stars
Scientific paper
Tables describing the evolution of stellar models with initial masses equal to 120, 85, 60, 40, 25, 20, and 15 solar masses are given for metallicities Z = 0.002, 0.005, 0.020, and 0.040. The evolution is followed from the zero-age sequence to the end of the central carbon-burning phase. The various model data are given here at corresponding evolutionary stages in each set of models. Together with up-to-date physical ingredients, these models are based on new opacity tables, which account for the fact that, at low metallicities, the abundances of several elements have nonsolar ratios with respect to iron. The present tables are a summary of more than 40,000 individual stellar models.
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