IAR 05382
INSTITUTO ARGENTINO DE RADIOASTRONOMIA
Unidad Ejecutora - UE
artículos
Título:
Radiation from hot accretion flows onto black holes
Autor/es:
FLORENCIA L. VIEYRO; EDUARDO M. GUTIÉRREZ; GUSTAVO ESTEBAN ROMERO
Revista:
Boletín de la Asociación Argentina de Astronomía
Editorial:
Comité Editorial de la Asociación Argentina de Astronomía
Referencias:
Año: 2019 vol. 61a
ISSN:
1669-9521
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.
