The effect of core overshooting and mass loss on the internal density concentration of main sequence stars

Details The effect of core overshooting and mass loss on the internal density concentration of main sequence stars The effect of core overshooting and mass loss on the internal density concentration of main sequence stars

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...244..319c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 2, April 1991, p. 319-326. CICYT-supported research.

Astronomy and Astrophysics

Astrophysics

20

Main Sequence Stars, Stellar Cores, Stellar Mass Ejection, Stellar Structure, Eclipsing Binary Stars, Stellar Evolution, Stellar Models, Stellar Temperature

Scientific paper

The paper presents a comparative study of internal structure constants for evolutionary models with overshooting and mass loss with respect to standard models. A total of five systems are studied at different evolutionary stages in order to establish the order of magnitude of the changes introduced in the internal density concentration by core overshooting. It is suggested that core shooting does not alter the general good agreement between theory and observations with respect to effective temperatures.

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