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...
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| 發表在: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要作者: | |
| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
Universidad Nacional Autónoma de México
2002
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| 主題: | |
| 在線閱讀: | https://www.redalyc.org/articulo.oa?id=57101327 |
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