Accretion vs. colliding wind models for the gamma-ray binary LS I + 61 303: An assessment
Context. LS I +61 303 is a puzzling Be/X-ray binary with variable gamma-ray emission up to TeV energies. The nature of the compact object and the origin of the high-energy emission are unclear. One family of models invokes particle acceleration in shocks from the collision between the B-star wind an...
Guardado en:
| Autores principales: | Romero, Gustavo Esteban, Okazaki, A. T., Orellana, Mariana Dominga, Owocki, S. P. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2007
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83335 |
| Aporte de: |
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