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Hydrodynamical Interaction between an Accretion Flow and a Stellar Wind

Molecular clouds in the interstellar medium suffer gravitational instabilitiesthat lead to the formation of one or multiple stars. A recently formed star insidea cold cloud communicates its gravitational force to the surrounding environmentand soon an accretion flow falling into the star develops. A...

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Bibliografiske detaljer
Udgivet i:Revista Mexicana de Astronomía y Astrofísica
Main Authors: S. Mendoza, J. Cantó, A. C. Raga
Format: Artigo
Sprog:Inglês
Udgivet: Universidad Nacional Autónoma de México 2004
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Online adgang:https://www.redalyc.org/articulo.oa?id=57140203
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