Mhd models for pne
A self-consistent scenario to explain the morphology of planetary nebulae ispresented. This scenario is consistent with the Galactic distribution of di erentnebular types. This work addresses several controversial features that appear inplanetary nebulae, which are easily solved by the inclusion of...
Guardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
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| Autores principales: | , , , , |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2000
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| Materias: | |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57100951 |
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