Radiative transfer approximations in stellar pulsation theory

Details Radiative transfer approximations in stellar pulsation theory Radiative transfer approximations in stellar pulsation theory

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8210970d&link_type=abstract

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Statistics

Computation

Celestial Bodies, Cepheid Variables, Heat Transfer, Pulse Modulation, Radioactivity, Stellar Models, Eddington Approximation, Mathematical Models, Radiant Cooling, Statistical Analysis, Variable Stars

Scientific paper

Pulsation theory is discussed in light of recent improvements in the
theory of radiative transfer and hydrodynamics with applications to
Cepheids, RR Lyrae, and W Virginis stars. It is concluded that the
variable Eddington method is computational fast and a complete transfer
approximation can be obtained.

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