Evolutionary sequences of stellar models with semiconvection and convective overshoot. I - Z = 0.008

Details Evolutionary sequences of stellar models with semiconvection and convective overshoot. I - Z = 0.008 Evolutionary sequences of stellar models with semiconvection and convective overshoot. I - Z = 0.008

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97..851a&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 4, p. 851-871.

Astronomy and Astrophysics

Astrophysics

162

Massive Stars, Stellar Convection, Stellar Cores, Stellar Evolution, Stellar Models, Hertzsprung-Russell Diagram, Nuclear Reactions, Stellar Composition, Stellar Interiors, Stellar Winds

Scientific paper

Two large grids of evolutionary models are presented for stars in the mass range 0.6 to 100 solar masses and chemical composition T = 0.25 and Z = 0.008. All evolutionary sequences are followed from zero age main sequence up to the stage of central carbon ignition of the thermally pulsing regime of the asymptotic giant branch phase. Massive stars are computed including the effect of mass loss by stellar wind over the entire evolutionary history, while low mass and intermediate mass stars are evolved at constant mass.

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