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Simulating the outer layers of rapidly rotating stars

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, no. 4 (2020): 5052-5059

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Abstract

This paper presents the results of a set of radiative hydrodynamic simulations of convection in the near-surface regions of a rapidly rotating star. The simulations use microphysics consistent with stellar models, and include the effects of realistic convection and radiative transfer. We find that the overall effect of rotation is to redu...More

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Robinson Frank
Robinson Frank
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