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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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autor: | |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2002
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57101327 |
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