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 \recombination{...
Zapisane w:
| Wydane w: | Revista Mexicana de Astronomía y Astrofísica |
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| 1. autor: | |
| Format: | Artigo |
| Język: | Inglês |
| Wydane: |
Universidad Nacional Autónoma de México
2001
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| Hasła przedmiotowe: | |
| Dostęp online: | https://www.redalyc.org/articulo.oa?id=57101017 |
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