Accretion Disks around Young Low Mass Stars
In the past decade, it has become clear that almost half of the low mass pre-main sequence stars are surrounded by disks, which are responsible for the observed infrared and optical-UV excess emission. The characterization of the structure of circumstellar disks is a crucial step towards understandi...
Guardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2001
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| Materias: | |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57101153 |
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