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Fliers as stagnation knots in planetary nebulae
We present an alternative model for the formation of fast low-ionization emission regions (FLIERs) in planetarynebulae. The model is able to account for many of their attendant characteristics and circumvent the problemsrelated to the collimation/formation mechanisms found in previous studies. In th...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2002
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57101329 |
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