Mass Loading by Proplyds of an O-Star Wind
Fuente:
Redalyc
Enregistré dans:
| Auteur principal: | |
|---|---|
| Format: | Artículo científico |
| Langue: | en |
| Publié: |
Universidad Nacional Autónoma de México
2002
|
| Sujets: | |
| Accès en ligne: | |
| Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
| _version_ | 1876444522416701440 |
|---|---|
| author | William J. Henney |
| author_facet | William J. Henney |
| contents | Mass Loading by Proplyds of an O-Star Wind William J. Henney S. J. Arthur F. García Arredondo Física, Astronomía y Matemáticas OUTFLOWS H II REGIONS STARS: WINDS HYDRODYNAMICS STARS: FOR MATION We present time-dependent, one-dimensional, numerical simulations of themass loading of the stellar wind from a high-mass star due to embedded proplyds.The simulations are tailored to the O star o1 Ori C in the Orion nebula, usingrealistic mass-loading rates taken from detailed studies of the Orion proplyds. Wefind significant dynamical effects on the wind due to the mass loading that can bedirectly compared with observational probes of the radial dependence of the windpressure. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57138106 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) Num.1 Vol.38 |
| format | Artículo científico |
| id | redalyc_57138106 |
| institution | Redalyc |
| language | en |
| publishDate | 2002 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Mass Loading by Proplyds of an O-Star Wind William J. Henney Física, Astronomía y Matemáticas OUTFLOWS H II REGIONS STARS: WINDS HYDRODYNAMICS STARS: FOR MATION Mass Loading by Proplyds of an O-Star Wind William J. Henney S. J. Arthur F. García Arredondo Física, Astronomía y Matemáticas OUTFLOWS H II REGIONS STARS: WINDS HYDRODYNAMICS STARS: FOR MATION We present time-dependent, one-dimensional, numerical simulations of themass loading of the stellar wind from a high-mass star due to embedded proplyds.The simulations are tailored to the O star o1 Ori C in the Orion nebula, usingrealistic mass-loading rates taken from detailed studies of the Orion proplyds. Wefind significant dynamical effects on the wind due to the mass loading that can bedirectly compared with observational probes of the radial dependence of the windpressure. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57138106 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) Num.1 Vol.38 |
| title | Mass Loading by Proplyds of an O-Star Wind |
| topic | Física, Astronomía y Matemáticas OUTFLOWS H II REGIONS STARS: WINDS HYDRODYNAMICS STARS: FOR MATION |
| url | https://www.redalyc.org/articulo.oa?id=57138106 |