Classical Cepheid Pulsation Models. III. The Predictable Scenario
Astrophysics
2009-10-31 v1
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
Cite
@article{arxiv.astro-ph/9908014,
title = {Classical Cepheid Pulsation Models. III. The Predictable Scenario},
author = {G. Bono and V. Castellani and M. Marconi},
journal= {arXiv preprint arXiv:astro-ph/9908014},
year = {2009}
}
Comments
24 pages, 1 latex file containing 6 tables, 10 postscript figures, accepted for publication on ApJ