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Velocity segregation in a clump-like outflow with a non-top hat velocity cross-section
High velocity clumps joined to the outflow source by emission with a “Hubble law” ramp of linearly increasing radial velocity vs. distance are observed in some planetary nebulae and in some outflows in star formation regions. We propose a simple model in which a “clump” is ejected from a source over...
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Veröffentlicht in: | Revista Mexicana de Astronomía y Astrofísica |
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Hauptverfasser: | , , , , |
Format: | Artigo |
Sprache: | Inglês |
Veröffentlicht: |
Universidad Nacional Autónoma de México
2021
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Online Zugang: | https://www.redalyc.org/articulo.oa?id=57171643002 |
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