Upload resources

Upload your works to SEDICI to increase its visibility and improve its impact

 

Transient high-energy flares from accreting black holes

Document type: Articulo

Abstract

We present a model for high-energy flares in accreting black holes based on the injection in a magnetized corona of a non-thermal population of relativistic particles. Coupled transport equations are solved for all species of particles and the electromagnetic and neutrino output is predicted for the case of Galactic black holes.

General information

Issue date: 2010
Document language: English
Journal: Proceedings of the International Astronomical Union; vol. 6, no. S275
Event: IAU Symposium 275 (Buenos Aires, Argentina, 13-17 September, 2010)
Origin: Facultad de Ciencias Astronómicas y Geofísicas; Instituto Argentino de Radioastronomía
Others identifiers: eid:2-s2.0-84882747423
ISSN: 1743-9213
Pages: 313-314
xmlui.dri2xhtml.METS-1.0.item-dc-subject: Galaxias ; Agujero negro
Subjects: Ciencias Astronómicas

Download Files

Thumbnail
Documento completo
Download file (129.0Kb) - PDF
 
Created: 3 de octubre de 2019
Available since: 3 de octubre de 2019
Please, use one of this identificators(URI) for cite o linking this item:
  • http://sedici.unlp.edu.ar/handle/10915/82628
  • https://doi.org/10.1017/S1743921310016261

    • This item appears in the following Collection(s)

    Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)