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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| Izdano u: | Revista Mexicana de Astronomía y Astrofísica |
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| Glavni autori: | , , |
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
Universidad Nacional Autónoma de México
2004
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| Teme: | |
| Online pristup: | https://www.redalyc.org/articulo.oa?id=57140203 |
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