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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...
Gorde:
| Argitaratua izan da: | Revista Mexicana de Astronomía y Astrofísica |
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| Egile nagusia: | |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Universidad Nacional Autónoma de México
2002
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| Gaiak: | |
| Sarrera elektronikoa: | https://www.redalyc.org/articulo.oa?id=57138108 |
| Etiketak: |
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