Stellar evolution with the Roxburgh criterion for convection

Details Stellar evolution with the Roxburgh criterion for convection Stellar evolution with the Roxburgh criterion for convection

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142..143d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 1, Jan. 1985, p. 143-149. Sponsorship: Fonds de la Recherche Fondamen

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Hertzsprung-Russell Diagram, Stellar Cores, Stellar Evolution, Stellar Luminosity, Stellar Structure, Supergiant Stars, Computational Astrophysics, Convection, Kinetic Energy, Star Clusters, Stellar Models

Scientific paper

The author shows that the Roxburgh criterion of convection gives an approximation of the flux of turbulent kinetic energy in a stellar convection zone. He presents evolutionary computations of 1.2 - 120 M_sun; stars, including overshooting from convective cores according to this criterion. He shows that these models represent the observational constraints much better than the classical models.

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