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...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , , , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2000
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57100951 |
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