Turbulent Convection in Pulsating Stars
arXiv:astro-ph/9901188
Abstract
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.)