Učitavanje...
Multiple Flow Interactions in a Proplyd Binary System I. The Interproplyd Shell
The Orion nebula proplyd 168{326 (LV 1) consists of a pair of photoevaporation flows, one from the circumstellar disk of each member of a protostellarbinary system. The two flows collide at mildly supersonic velocities, producing adense interproplyd shell bounded by two weak shocks, while further in...
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| Izdano u: | Revista Mexicana de Astronomía y Astrofísica |
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| Glavni autor: | |
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
Universidad Nacional Autónoma de México
2002
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| Teme: | |
| Online pristup: | https://www.redalyc.org/articulo.oa?id=57138108 |
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