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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| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2008
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57116159051 |
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