English

Nonlinear Beat Cepheid Models

Astrophysics 2016-08-30 v2

Abstract

The numerical hydrodynamic modelling of beat Cepheid behavior has been a longstanding quest in which purely radiative models have failed miserably. We find that beat pulsations occur naturally when turbulent convection is accounted for in our hydrodynamics codes. The development of a relaxation code and of a Floquet stability analysis greatly facilitates the search for and analysis of beat Cepheid models. The conditions for the occurrence of beat behavior can be understood easily and at a fundamental level with the help of amplitude equations. Here a discriminant D arises whose sign decides whether single mode or double mode pulsations can occur in a model, and this D depends only on the values of the nonlinear coupling coefficients between the fundamental and the first overtone modes. For radiative models D is always found to be negative, but with sufficiently strong turbulent convection its sign reverses.

Keywords

Cite

@article{arxiv.astro-ph/9804111,
  title  = {Nonlinear Beat Cepheid Models},
  author = {Z. Kollath and J. P. Beaulieu and J. R. Buchler and P. Yecko},
  journal= {arXiv preprint arXiv:astro-ph/9804111},
  year   = {2016}
}

Comments

5 pages, incl. 4 figs - apj lett, accepted may 18, 1998