High-energy signatures of binary systems of supermassive black holes

Context. Binary systems of supermassive black holes are expected to be strong sources of long gravitational waves prior to merging. These systems are good candidates to be observed with forthcoming space-borne detectors. Only a few of these systems, however, have been firmly identified to date. Ai...

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Detalles Bibliográficos
Autores principales:	Romero, Gustavo Esteban, Vila, Gabriela Soledad, Pérez, Daniela
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2016
Materias:	Ciencias Astronómicas Accretion, accretion disks Galaxies: active Galaxies: jets Radiation mechanisms: non-thermal
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/86716
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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