Emission lines from Jets in planetary nebulae
Emission line proles from collimated high-velocity outows or jets in planetary nebulae (PNe) have diversecharacteristics that indicate the inuence of binary cores and magnetic connement mechanisms in their origin.In this contribution, a number of cases are presented that exemplify the complexity of...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 第一著者: | |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2002
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57101327 |
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