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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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2010
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57115706045 |
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