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Nonlinear Survey of RRd Models
Published online by Cambridge University Press: 12 April 2016
Abstract
We used our nonlinear hydrodynamical code with turbulent convection to model RR Lyrae stars. In some regime this approach produces double-mode solutions. We investigated series of models with different parameters (metallicity, luminosity, etc.). Our goal was to estimate the width of the double-mode region. The resulting tendencies can be directly compared with observational properties.
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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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