High-energy astrophysics on compact objects: accretion on all scales

La emisión gamma es la evidencia mas fuerte de que procesos no-térmicos tienen lugar en una fuente astrofísica. Estos procesos son el resultado de la presencia de partículas relativistas que interaccionan con los diferentes campos, como el campo magnético, de radiación y de materia fría. En este tra...

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Detalles Bibliográficos
Autor principal:	Vieyro, Florencia Laura
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2019
Materias:	Ciencias Astronómicas radiation mechanisms: non-thermal gamma rays: general stars: black holes
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/170362
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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