On the dependence of some helium shell flash characteristics on core mass

Details On the dependence of some helium shell flash characteristics on core mass On the dependence of some helium shell flash characteristics on core mass

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240..196h&link_type=abstract

Astrophysical Journal, Part 1, vol. 240, Aug. 15, 1980, p. 196-202. U.S.-Israel Binational Science Foundation

Computer Science

Numerical Analysis

Helium, Stellar Atmospheres, Stellar Evolution, Stellar Luminosity, Stellar Mass, Stellar Structure, Cores, Numerical Analysis, Stellar Temperature

Scientific paper

A theoretical derivation of the intershell mass-core mass relation of
Paczynski is attempted. Formulas developed by Sugimoto and Fujimoto
(1978) are extended to less massive cores with m(c) not greater than 1.

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