Ionized photoevaporation flows in h II regions and PNe
Fuente:
Redalyc
Saved in:
| Main Author: | |
|---|---|
| Format: | Artículo científico |
| Language: | en |
| Published: |
Universidad Nacional Autónoma de México
2001
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1876429735650656256 |
|---|---|
| author | W. J. Henney |
| author_facet | W. J. Henney |
| contents | Ionized photoevaporation flows in h II regions and PNe W. J. Henney Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE 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{dominated"ows that predominate in H II regions. The general properties of such ows arediscussed, with particular reference to recent results on the Orion proplyds and theHelix knots. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101017 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.10 |
| format | Artículo científico |
| id | redalyc_57101017 |
| institution | Redalyc |
| language | en |
| publishDate | 2001 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Ionized photoevaporation flows in h II regions and PNe W. J. Henney Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE Ionized photoevaporation flows in h II regions and PNe W. J. Henney Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE 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{dominated"ows that predominate in H II regions. The general properties of such ows arediscussed, with particular reference to recent results on the Orion proplyds and theHelix knots. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101017 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.10 |
| title | Ionized photoevaporation flows in h II regions and PNe |
| topic | Física, Astronomía y Matemáticas H II REGIONS PLANETARY NEBULAE |
| url | https://www.redalyc.org/articulo.oa?id=57101017 |