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Ionized photoevaporation flows in h II regions and PNe
From proplyds to champagne ows, spanning 4 orders of magnitude in sizeand density, photoevaporation ows are ubiquitous in H II regions. Such ows arealso found in planetary nebulae, in the form of cometary knots, although in this casethe ows are often \advection{dominated", unlike the \recombina...
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| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor Principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2001
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| Assuntos: | |
| Acceso en liña: | https://www.redalyc.org/articulo.oa?id=57101017 |
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