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...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2000
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57100951 |
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