EXCITING NEW VISTAS ON THE FORMATION OF HIGH MASS STARS
High mass young stellar objects (YSOs) are usually deeply embedded in their natal environment which can be penetrated only at wavelengths beyond the mid infrared. However, taking advantage of "curtain lifting" stellar winds and ionizing photons from neighbouring SpT O main sequence stars and making...
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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
2008
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57116159051 |
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