Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...96..255c&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 96, no. 2, p. 255-268.
Astronomy and Astrophysics
Astrophysics
175
Eclipsing Binary Stars, Stellar Evolution, Stellar Interiors, Stellar Models, Abundance, Metallicity, Stellar Composition
Scientific paper
The present stellar evolutionary models, which include internal structure constants, employ the most recent input physics and use the Rogers and Iglesias (1992) opacities, in conjunction with the recent lower-temperature computations of Alexander (1992). The primary changes those obtained concern the solar He content and mixing-length parameter. The new models exhibit a general tendency to be cooler and more centrally concentrated in mass than previous computation results for masses where apsidal motion is observed.
Claret Antonio
Gimenez Alvaro
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