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SPATIAL DISTRIBUTION OF STELLAR ROTATIONAL AXES FROM BE STARS

In order to know the distribution of rotational velocities of Be stars, a standard assumption is used, namelythat the rotational axes are uniformed distributed. We use here polarimetric projected angles data from almost500 Be stars and we make a statistical analysis. Furthermore we perform a Monte-C...

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Bibliografski detalji
Izdano u:Revista Mexicana de Astronomía y Astrofísica
Glavni autori: M. Curé, A. Christen, Th. Rivinius, D. F. Rial
Format: Artigo
Jezik:Inglês
Izdano: Universidad Nacional Autónoma de México 2010
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Online pristup:https://www.redalyc.org/articulo.oa?id=57115706045
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