Classical Cepheid Pulsation Models. III. The Predictable Scenario
- 20 January 2000
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 529 (1) , 293-317
- https://doi.org/10.1086/308263
Abstract
Within the current uncertainties in the treatment of the coupling between pulsation and convection, limiting amplitude, nonlinear, convective models appear the only viable approach for providing theoretical predictions about the intrinsic properties of radial pulsators. In this paper we present the results of a comprehensive set of Cepheid models computed within such theoretical framework for selected assumptions on their original chemical composition.Keywords
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