A demonstration calculation of self-consistent stellar models with convective cores

Details A demonstration calculation of self-consistent stellar models with convective cores A demonstration calculation of self-consistent stellar models with convective cores

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988amjph..56...68l&link_type=abstract

American Journal of Physics, Volume 56, Issue 1, pp. 68-72 (1988).

Physics

1

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

A quick procedure for calculating self-consistent stellar models is described. The procedure involves the matching of radiative stellar envelope solutions to convective core solutions. The core is assumed to have the adiabatic temperature gradient. This procedure was developed for demonstrating stellar model calculations in upper year undergraduate astrophysics courses.

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