info:eu-repo/semantics/article
Radiation from hot accretion flows onto black holes
Fecha
2019-08Registro en:
Gutiérrez, Eduardo Mario; Vieyro, Florencia Laura; Romero, Gustavo Esteban; Radiation from hot accretion flows onto black holes; Asociación Argentina de Astronomía; Boletín de la Asociación Argentina de Astronomía; 61A; 8-2019
1669-9521
CONICET Digital
CONICET
Autor
Gutiérrez, Eduardo Mario
Vieyro, Florencia Laura
Romero, Gustavo Esteban
Resumen
The hot accretion flows upon black holes are usually optically thin two-temperature plasmas in which electrons can achieve temperatures up to , producing radiation via synchrotron, bremsstrahlung and inverse Compton, and the ions can reach temperatures up to . The hottest ions might produce gamma emission through proton-proton interactions. In this work, we considered a particular model of a hot accretion flow and estimate the spectral energy distributions produced by both species of particles.