Stellar evolutionary models from the zero-age main sequence to the first thermal pulse

Details Stellar evolutionary models from the zero-age main sequence to the first thermal pulse Stellar evolutionary models from the zero-age main sequence to the first thermal pulse

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apjs...76..215l&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 76, May 1991, p. 215-357.

Physics

62

Main Sequence Stars, Stellar Evolution, Stellar Models, Stellar Structure, Asymptotic Giant Branch Stars, Convection Currents, Metallicity, Stellar Interiors, Stellar Mass, Stellar Temperature

Scientific paper

Detailed numerical tabulations are presented of 32 stellar evolutionary sequences extending from either the zero-age main-sequence or the zero-age horizontal branch, and through to the occurrence of thermal pulses on the asymptotic giant branch. The models span a range of 1-3 solar masses (except for one of 4-solar mass and one 5-solar mass model) and cover metallicities of Z = 0.02, 0.01, 0.006, 0.003, and 0.001, each with Y = 0.20 and 0.30. These models can be used for various stellar population studies, and as a comparison between rival calculations with different input physics.

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