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3D hydrodynamic simulations of massive main-sequence stars. III. The effect of radiation pressure and diffusion leading to a 1D equilibrium model

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Mao, Huaqing, Woodward, Paul, Herwig, Falk, Denissenkov, Pavel A., Blouin, Simon, Thompson, William, McDermott, Benjamin
Natura:	Preprint
Pubblicazione:	2023
Soggetti:	Solar and Stellar Astrophysics
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

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