Gamma-ray variability from stellar wind porosity in microquasar systems
In the subclass of high-mass X-ray binaries known as “microquasars,” relativistic hadrons in the jets launched by the compact object can interact with cold protons from the star's radiatively driven wind, producing pions that then quickly decay into gamma rays. Since the resulting gamma-ray emi...
Guardado en:
| Autores principales: | Owocki, Stanley P., Romero, Gustavo Esteban, Townsend, Richard H. D., Araudo, Anabella Teresa |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2010
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/101794 https://ri.conicet.gov.ar/11336/6309 http://aspbooks.org/custom/publications/paper/422-0049.html |
| Aporte de: |
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