INVESTIGATING BE STAR DISKS USING LONG-BASELINE INTERFEROMETRY
Be stars form a subclass of B-type stars, where the stars possess gaseous disk-like structures. Historically, the presence of a disk was detected through line emission present in the spectrum, or through IR excess detected in the spectral energy distribution originating from these sources. However,...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| 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=57115706030 |
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