Thermal imbalance effects on pulsational stability in stellar models

Details Thermal imbalance effects on pulsational stability in stellar models Thermal imbalance effects on pulsational stability in stellar models

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.112..185c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 112, no. 1, May 1985, p. 185-192.

Astronomy and Astrophysics

Astrophysics

Nonequilibrium Thermodynamics, Stellar Models, Stellar Oscillations, Stellar Temperature, Adiabatic Conditions, Eigenvalues, Point Sources, Roche Limit

Scientific paper

The treatment followed by Cox et al. (1973) for the estimation of the effects of termal imbalance on the pulsational stability of stars is applied to Roche and point source (Chandrika Prashad) model. The calculations suggest that the eigenvalues obtained for the above model are correct to 0(tff/ts). The expressions for stability coefficients and corresponding eigenfunctions for the stars in thermal imbalance for the above models have also been derived.

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