Radiation from hot accretion flows onto black holes

Los flujos de acreción calientes que tienen lugar alrededor de agujeros negros consisten en plasmas ópticamente delgados, en donde los electrones pueden alcanzar temperaturas de hasta 10¹⁰ K y producir radiación por sincrotrón, bremsstrahlung y Compton inverso, y los iones pueden alcanzar temperatur...

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Detalles Bibliográficos
Autores principales:	Gutiérrez, Eduardo Mario, Vieyro, Florencia Laura, Romero, Gustavo Esteban
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2019
Materias:	Ciencias Astronómicas stars: black holes accretion, accretion disks radiation mechanisms: thermal
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/170367
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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