Coupling coefficients of pulsation for radiative stellar models

Details Coupling coefficients of pulsation for radiative stellar models Coupling coefficients of pulsation for radiative stellar models

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44..101t&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 2, 1992, p. 101-107.

Statistics

Computation

10

Computational Astrophysics, Coupling Coefficients, Stellar Models, Stellar Oscillations, Stellar Radiation, Adiabatic Conditions, Cepheid Variables, Entropy

Scientific paper

The second-order theory of coupling is discussed regarding the radial pulsation of radiative stellar models, while taking nonadiabatic effects into consideration. Numerical values are given for model classical cepheids. Adiabatic coupling coefficients are changed slightly when convection is ignored. The entropy changes near the stellar surface increase the strength of coupling.

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