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...
Uloženo v:
| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Hlavní autoři: | , , , , |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2000
|
| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57100951 |
| Tagy: |
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!
|