STUDYING THE PHYSICAL CONDITIONS IN BE STAR DISKS USING NON-LTE RADIATIVE TRANSFER CODES
Classical Be stars are rapidly rotating, massive stars that exhibit several distinct observational characteristics due to the presence of thin disks of gas concentrated in the stars equatorial plane. In order to understand the mechanisms that govern the development of these circumstellar disks, we u...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2010
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57115706031 |
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