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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Detalles Bibliográficos
Autores principales: Venero, R.O.J., Cure, M., Cidale, L.S., Rial, D.F.
Formato: CONF
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p94_Venero
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id todo:paper_14052059_v33_n_p94_Venero
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spelling todo:paper_14052059_v33_n_p94_Venero2023-10-03T16:12:58Z Axisymmetric stellar wind models Venero, R.O.J. Cure, M. Cidale, L.S. Rial, D.F. 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. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar 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.
format CONF
author Venero, R.O.J.
Cure, M.
Cidale, L.S.
Rial, D.F.
spellingShingle Venero, R.O.J.
Cure, M.
Cidale, L.S.
Rial, D.F.
Axisymmetric stellar wind models
author_facet Venero, R.O.J.
Cure, M.
Cidale, L.S.
Rial, D.F.
author_sort Venero, R.O.J.
title 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
url http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p94_Venero
work_keys_str_mv AT veneroroj axisymmetricstellarwindmodels
AT curem axisymmetricstellarwindmodels
AT cidalels axisymmetricstellarwindmodels
AT rialdf axisymmetricstellarwindmodels
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