Thermal response of stellar envelopes during nonradial pulsations

Details Thermal response of stellar envelopes during nonradial pulsations Thermal response of stellar envelopes during nonradial pulsations

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...285..778p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 285, Oct. 15, 1984, p. 778-783.

Statistics

Computation

4

Stellar Envelopes, Stellar Models, Stellar Oscillations, Computational Astrophysics, Eigenvalues, Linear Energy Transfer (Let), Nonadiabatic Theory, Propagation Velocity, Stellar Temperature, Sturm-Liouville Theory, Thermodynamics

Scientific paper

The response of spherical stellar envelopes in hydrostatic and thermal balance to nonradial thermal distributions is outlined. Because of the nature of the initial model, the governing equations yield an operator that is almost identical to the radial case. The use of propagation velocities to estimate the nonadiabatic effects in a pulsation is demonstrated.

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