Stagnation knots in planetary nebulae
We present an alternative model for the formation of fast low-ionization emission regions (FLIERs) in planetarynebulae. In this model, a concave bow-shock structure is formed as a result of a reduced momentum ow alongthe symmetry axis of a stellar wind. FLIERS are formed from the shocked ambient med...
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| Publié dans: | Revista Mexicana de Astronomía y Astrofísica |
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| Auteurs principaux: | , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
Universidad Nacional Autónoma de México
2002
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| Sujets: | |
| Accès en ligne: | https://www.redalyc.org/articulo.oa?id=57112052 |
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