Outflows, jets and shocks in the orion nebula
The rich young cluster of stars associated with the Orion Nebula provides aunique laboratory for the study of plasma phenomena. We see ve types of owsand shocks. Photoablation outow from the proplyds nearest 1Ori C form nearlystationary shocks with the high velocity wind from that star. Microjets, w...
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| Gepubliceerd in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hoofdauteurs: | , |
| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Universidad Nacional Autónoma de México
2000
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| Onderwerpen: | |
| Online toegang: | https://www.redalyc.org/articulo.oa?id=57100948 |
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