A detailed grid of evolutionary stellar models during hydrogen burning phases

Details A detailed grid of evolutionary stellar models during hydrogen burning phases A detailed grid of evolutionary stellar models during hydrogen burning phases

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...81....1c&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 81, no. 1, Nov. 1989, p. 1-35. Research supported by CAICYT.

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66

Computational Astrophysics, Eclipsing Binary Stars, Nuclear Astrophysics, Stellar Evolution, Stellar Models, Chemical Composition, Runge-Kutta Method, Stellar Interiors, Stellar Mass

Scientific paper

Stellar evolution calculations are conducted to improve and extend the comparison of empirical stellar data with theoretical predictions. The calculations are made for five chemical compositions around the Ross-Aller mixture. The grid of models covers a mass range of 0.6-25 solar masses from zero-age main sequence to evolutionary phases corresponding to the depletion of hydrogen in the core. An average of 160 models were generated per evolutionary track for the standard chemical composition, each including the computation of about 300 layers inside the star.

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