THE EXPANSION OF A STELLAR WIND BUBBLE WITHIN A NON-SINGULAR, STRATIFIED CORE

We study analytically the expansion of a non-radiative bubble (driven by the wind from a massive star) into an environment with a non-singular, self-gravitating isothermal sphere density stratification. We derive the equation of motion forthe outer radius of the bubble (using the assumptions of th...

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Udgivet i:Revista Mexicana de Astronomía y Astrofísica
Main Authors: J. C. Rodríguez-Ramírez, A. C. Raga
Format: Artigo
Sprog:Inglês
Udgivet: Universidad Nacional Autónoma de México 2012
Fag:
Física, Astronomía y Matemáticas
ISM: evolution
stars: formation
ISM: kinematics and dynamics
Online adgang:https://www.redalyc.org/articulo.oa?id=57124423007
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