Driving and damping mechanisms in hybrid pressure-gravity modes pulsators
Solar and Stellar Astrophysics
2015-05-13 v1
Abstract
We study the energetic aspects of hybrid pressure-gravity modes pulsations. The case of hybrid beta Cephei-SPB pulsators is considered with special attention. In addition to the already known sensitivity of the driving mechanism to the heavy elements mixture (mainly the iron abundance), we show that the characteristics of the propagation and evanescent regions play also a major role, determining the extension of the stable gap in the frequency domain between the unstable low order pressure and high order gravity modes. Finally, we consider the case of hybrid delta Sct-gamma Dor pulsators.
Keywords
Cite
@article{arxiv.0907.2636,
title = {Driving and damping mechanisms in hybrid pressure-gravity modes pulsators},
author = {M. -A Dupret and A. Miglio and J. Montalban and A. Grigahcene and A. Noels},
journal= {arXiv preprint arXiv:0907.2636},
year = {2015}
}
Comments
7 pages, 9 figures, in the proceedings of the Helas II Conference: "Helioseismology, Asteroseismology and MHD Connections", Goettingen, August 2007