Author:
Szabó R.,Kolláth Z.,Csubry Z.,Buchler J. R.
Abstract
AbstractWe 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.
Publisher
Cambridge University Press (CUP)
Cited by
2 articles.
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1. Hydrodynamical Modeling of Double-Mode Pulsation;International Astronomical Union Colloquium;2000
2. The Instability Strip of M3;International Astronomical Union Colloquium;2000