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Turbulent Convection in Pulsating Stars

J. Robert Buchler·Philip Yecko·Zoltan Kollath·Marie-Jo Goupil
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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.

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J. Robert Buchler, Philip Yecko, Zoltan Kollath, Marie-Jo Goupil. 1999-01-14. Turbulent Convection in Pulsating Stars. https://arxiv.org/abs/astro-ph/9901188

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