Upload resources

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

 

Show simple item record

dc.date.accessioned 2019-10-03T16:36:22Z
dc.date.available 2019-10-03T16:36:22Z
dc.date.issued 2010
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82628
dc.description.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. en
dc.format.extent 313-314 es
dc.language en es
dc.subject Galaxias es
dc.subject Agujero negro es
dc.title Transient high-energy flares from accreting black holes en
dc.type Articulo es
sedici.identifier.other eid:2-s2.0-84882747423 es
sedici.identifier.other doi:10.1017/S1743921310016261 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Vieyro, Florencia Laura es
sedici.creator.person Romero, Gustavo Esteban es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
mods.originInfo.place Instituto Argentino de Radioastronomía es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event IAU Symposium 275 (Buenos Aires, Argentina, 13-17 September, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 6, no. S275 es


Download Files

Thumbnail
Documento completo
Download file (129.0Kb) - PDF

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)