Nonthermal processes in hot accretion flows onto supermassive black holes: an inhomogeneous model

Context. Many low-redshift active galactic nuclei harbor a supermassive black hole accreting matter at low or medium rates. At such rates, the accretion flow usually consists of a cold optically thick disk, plus a hot, low density, collisionless corona. In the latter component, charged particles can...

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Detalles Bibliográficos
Autores principales:	Gutiérrez, Eduardo Mario, Vieyro, Florencia Laura, Romero, Gustavo Esteban
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2021
Materias:	Ciencias Astronómicas Relativistic processes Radiation mechanisms: nonthermal Black hole physics Accretion, accretion disks Galaxies: active
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/125584
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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