Stellar evolution. IV - Evolution of a star of 1.5 solar masses from the main-sequence to the red-giant branch with and without overshooting from convective core

Details Stellar evolution. IV - Evolution of a star of 1.5 solar masses from the main-sequence to the red-giant branch with and without overshooting from convective core Stellar evolution. IV - Evolution of a star of 1.5 solar masses from the main-sequence to the red-giant branch with and without overshooting from convective core

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....43...61m&link_type=abstract

Astronomy and Astrophysics, vol. 43, no. 1, Sept. 1975, p. 61-69.

Astronomy and Astrophysics

Astrophysics

26

Main Sequence Stars, Star Clusters, Stellar Evolution, Astronomical Models, Convective Flow, Mixing Length Flow Theory, Stellar Structure

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1975A&A....43...61M

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