Gamma-ray emission from massive young stellar objects
Context.Massive stars form in dense and massive molecular cores. The exact formation mechanism is unclear, but it is possible that some massive stars are formed by processes similar to those that produce the low-mass stars, with accretion/ejection phenomena occurring at some point of the evolution o...
Guardado en:
| Autores principales: | Araudo, Anabella Teresa, Romero, Gustavo Esteban, Bosch Ramon, V., Paredes, J. M. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2007
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83146 |
| Aporte de: |
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