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Hydrodynamical Modeling of Double-Mode Pulsation
Published online by Cambridge University Press: 12 April 2016
Abstract
The hydrodynamical modeling of steady double-mode (DM) pulsations has been a long-standing quest. Recent improvements in turbulent-convective pulsation codes provide a natural way to calculate nonlinear DM oscillations. The eddy viscosity plays a crucial role in these models. We present models both for RRd and beat Cepheid variables and for different chemical compositions. Simple nonresonant amplitude equations capture the DM phenomenon, giving an overview of modal selection on the HR diagram.
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- Part 5. Theoretical Models of Classical Pulsating Stars
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- Copyright © Astronomical Society of the Pacific 2000
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