Evento

Gamma-ray flares from black hole coronae

Vieyro, Florencia LauraIcon ; Romero, Gustavo EstebanIcon
Colaboradores: Rieger , Frank M.; van Eldik, Christopher; Hofmann, Werner
Tipo del evento: Congreso
Nombre del evento: 25th Texas Symposium on Relativistic Astrophysics
Fecha del evento: 06/12/2010
Institución Organizadora: Max-Planck-Institut für Kernphysik;
Título del Libro: Proceedings of Science
Título de la revista: Proceedings of Science
Editorial: Sissa Medialab
ISSN: 1824-8039
Idioma: Inglés
Clasificación temática:

Resumen

We present results of a study of non-thermal, time-dependent particle injection in a corona around an accreting black hole. We model the spectral energy distribution of high-energy flares in this scenario. We consider particle interactions with magnetic, photon and matter fields in the black hole magnetosphere. Transport equations are solved for all species of particles and the electromagnetic output is predicted. Photon annihilation is taken into account for the case of systems with early-type donor stars.
Palabras clave: Black holes , Early-type stars
 
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Licencia
info:eu-repo/semantics/openAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/222532
URL: https://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=123
URL: https://www.mpi-hd.mpg.de/texas2010/pages/news.php
Colecciones
Eventos(IAR)
Eventos de INST.ARG.DE RADIOASTRONOMIA (I)
Citación
Gamma-ray flares from black hole coronae; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania; 2010; id. 174, 1-7
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