Relativistic particle content in the most massive colliding-wind binary in the Galaxy
The wind-collision region of the system HD 93129A was recently resolved. This system is the most massive known binary in our Galaxy. We aim to gain insight into the physics taking place in such a system, particularly in the acceleration process(es). We explored the broadband non-thermal emission for...
Guardado en:
| Autores principales: | Palacio, Santiago del, Romero, Gustavo Esteban, Bosch-Ramon, Valentí, Benaglia, Paula |
|---|---|
| Formato: | Objeto de conferencia |
| Lenguaje: | Inglés |
| Publicado: |
2015
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/168087 |
| Aporte de: |
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