Classical Cepheid Pulsation Models. III. The Predictable Scenario
天体物理学
2009-10-31 v1
摘要
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.
引用
@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}
}
备注
24 pages, 1 latex file containing 6 tables, 10 postscript figures, accepted for publication on ApJ