Towards a self-consistent model of the convective core boundary in upper main sequence stars. Part I: 2.5D and 3D simulations

Fuente: arXiv

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Bibliographic Details
Main Authors:	Andrassy, R., Leidi, G., Higl, J., Edelmann, P. V. F., Schneider, F. R. N., Roepke, F. K.
Format:	Preprint
Published:	2023
Subjects:	Solar and Stellar Astrophysics Fluid Dynamics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2307.04068