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Nonlinear Pulsations of Convective Stellar Models

Published online by Cambridge University Press:  12 April 2016

J. Robert Buchler
J. Robert Buchler*
Affiliation:
Physics Department, University of Florida, Gainesville, FL 32611, USA

Abstract

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We review the numerical modeling of the nonlinear pulsations of classical variable stars with hydro-codes that include the effects of turbulent convection. Despite their simplicity these turbulent convective recipes appear to remove many of the difficulties that radiative codes faced. In particular, the numerical modeling of double mode pulsations has become possible.

Type
Part 5. Theoretical Models of Classical Pulsating Stars
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 343 - 355
Copyright
Copyright © Astronomical Society of the Pacific 2000

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