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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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Dettagli Bibliografici
Autori principali:	Andrassy, R., Leidi, G., Higl, J., Edelmann, P. V. F., Schneider, F. R. N., Roepke, F. K.
Natura:	Preprint
Pubblicazione:	2023
Soggetti:	Solar and Stellar Astrophysics Fluid Dynamics
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

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