Non-radial secular stability of the hydrogen burning shell in stars of 1.1 and 8 solar masses

Details Non-radial secular stability of the hydrogen burning shell in stars of 1.1 and 8 solar masses Non-radial secular stability of the hydrogen burning shell in stars of 1.1 and 8 solar masses

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....46..313g&link_type=abstract

Astronomy and Astrophysics, vol. 46, no. 2, Jan. 1976, p. 313-316.

Astronomy and Astrophysics

Astrophysics

3

Secular Variations, Stellar Atmospheres, Stellar Evolution, Eigenvalues, Main Sequence Stars, Nuclear Reactions, Perturbation Theory, Stellar Mass

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976A&A....46..313G

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