Turbulent Convection in Pulsating Stars

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We review recent results of stellar pulsation modelling that show that even very simple one-dimensional models for time dependent turbulent energy diffusion and convection provide a substantial improvement over purely radiative models.
Workshop on Stellar Structure: Theory and Tests of Convective Energy Transport, Granada, SPAIN, 1998 (to be published in the ASP Conf. Ser.)

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/13689

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9901188
 http://arxiv.org/abs/astro-ph/9901188

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arXiv