Stellar evolution with the Roxburgh criterion for convection.

198513 citationsJournal Article

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Abstract

On montre que le critere de convection de Roxburgh donne une approximation du flux d'energie cinetique turbulente dans une zone de convection stellaire. On presente les calculs d'evolution d'etoiles de 12 a 120 M○.

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Stellar, planetary, and galactic studies Solar and Space Plasma Dynamics Astronomy and Astrophysical Research

Publication Details

Volume 142, Issue 1, pp. 143-149

Field-Weighted Citation Impact: 5.39

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Stellar evolution with the Roxburgh criterion for convection.

Authors

Abstract

Topics & Keywords

Publication Details