Static stellar models with helium cores

Details Static stellar models with helium cores Static stellar models with helium cores

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....53..419l&link_type=abstract

Astronomy and Astrophysics, vol. 53, no. 3, Dec. 1976, p. 419-429.

Other

2

Helium, Nuclear Fusion, Stellar Models, Stellar Structure, Temperature Distribution, Chemical Composition, Curve Fitting, Isothermal Processes, Stellar Envelopes, Stellar Mass, Ubv Spectra

Scientific paper

The properties of static stellar models with helium cores are discussed with particular emphasis on those features which produce multiple solutions. A stellar model is obtained by fitting core solutions to envelope solutions in a U-V plane. The large number of possible solutions which have been found in earlier numerical computations (up to nine different solutions for a model of given mass and chemical composition) can be explained by the various intersections of the envelope and the core fit-curves, and the typical features of the fit-curves can in turn be identified with the corresponding physical effects

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