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...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2000
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57100948 |
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