Axisymmetric stellar wind models
The effects of stellar rotation on the shape of a star are included in the radiation-driven wind theory in order to study their influence upon disk formation in Be stars. For this purpose, we consider a rotationally oblated star and obtain the line force parameters consistently with the hydrodynamic...
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2008
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v33_n_p94_Venero http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p94_Venero |
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paper:paper_14052059_v33_n_p94_Venero |
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paper:paper_14052059_v33_n_p94_Venero2023-06-08T16:13:21Z Axisymmetric stellar wind models The effects of stellar rotation on the shape of a star are included in the radiation-driven wind theory in order to study their influence upon disk formation in Be stars. For this purpose, we consider a rotationally oblated star and obtain the line force parameters consistently with the hydrodynamic momentum equations. We discuss the influence of the rotation and the bi-stability mechanism in the formation of a two-component wind (fast wind in polar latitudes and slow wind in equatorial regions). © 2008: Instituto de Astronomía. 2008 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v33_n_p94_Venero http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p94_Venero |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| description |
The effects of stellar rotation on the shape of a star are included in the radiation-driven wind theory in order to study their influence upon disk formation in Be stars. For this purpose, we consider a rotationally oblated star and obtain the line force parameters consistently with the hydrodynamic momentum equations. We discuss the influence of the rotation and the bi-stability mechanism in the formation of a two-component wind (fast wind in polar latitudes and slow wind in equatorial regions). © 2008: Instituto de Astronomía. |
| title |
Axisymmetric stellar wind models |
| spellingShingle |
Axisymmetric stellar wind models |
| title_short |
Axisymmetric stellar wind models |
| title_full |
Axisymmetric stellar wind models |
| title_fullStr |
Axisymmetric stellar wind models |
| title_full_unstemmed |
Axisymmetric stellar wind models |
| title_sort |
axisymmetric stellar wind models |
| publishDate |
2008 |
| url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v33_n_p94_Venero http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p94_Venero |
| _version_ |
1768543719001161728 |