Tables of isochrones computed from stellar models with mass loss and overshooting

Details Tables of isochrones computed from stellar models with mass loss and overshooting Tables of isochrones computed from stellar models with mass loss and overshooting

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...89..451m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 89, no. 3, Sept. 1991, p. 451-467.

Astronomy and Astrophysics

Astrophysics

116

Main Sequence Stars, Star Clusters, Stellar Mass Ejection, Stellar Models, Wolf-Rayet Stars, Abundance, Hertzsprung-Russell Diagram, Stellar Evolution

Scientific paper

New sets of isochrones were computed from stellar models for Population I stars, taking into account the effects of mass loss and core overshooting. The star models used are those of Maeder and Meynet (1989) for stars having an initial mass inferior to 12 solar masses, and those of Maeder (1990) for the more massive stars. A comparison with observations showed the need of overshooting for stars with an initial mass superior to 1.6 solar mass. The new sets predict large changes for the age determinations.

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