The effect of convection on pulsational stability

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A review on the current state of mode physics in classical pulsators is presented. Two, currently in use, time-dependent convection models are compared and their applications on mode stability are discussed with particular emphasis on the location of the Delta Scuti instability strip.
Accepted for publication in CoAst (invited paper), 9 pages, 4 figures

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/172687

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0810.5228
 http://arxiv.org/abs/0810.5228

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arXiv