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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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2002 |
| País: | México |
| Institución: | Universidad Nacional Autónoma de México |
| Repositorio: | Redalyc-UNAM |
| OAI Identifier: | oai:redalyc.org:57101327 |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57101327 |
| Access Level: | acceso abierto |
| Palabra clave: | Física, Astronomía y Matemáticas PLANETARY NEBULAE ISM: JETS AND OUTFLOWS |
| Sumario: | 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 these outows in PNe.C |
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