Predictions of Very High Energy gamma-ray fluxes for three Active Galactic Nuclei
| dc.creator | Lenain, Jean-Philippe | |
| dc.date | 2007-09-15 | |
| dc.date.accessioned | 2026-07-07T08:29:49Z | |
| dc.date.available | 2026-07-07T08:29:49Z | |
| dc.description | M87 is the first extragalactic source detected at the TeV that is not a blazar. To account for the recent observations of M87 made by the High Energy Stereoscopic System (H.E.S.S.) telescope array, we developed a new multi-blob synchrotron self-Compton model. In the framework of this model, we present here the predictions for the very high energy emission of three active galactic nuclei with extended optical or X-ray jets which could be misaligned blazars, namely Cen A, PKS 0521-36 and 3C 273. | |
| dc.description | 4 pages, 3 figures; to appear in "SF2A 2007 proceedings", eds. J. Bouvier, A. Chalabaev and C. Charbonnel | |
| dc.identifier | https://arxiv.org/abs/0709.2400 | |
| dc.identifier | http://arxiv.org/abs/0709.2400 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/138076 | |
| dc.subject | Astrophysics | |
| dc.title | Predictions of Very High Energy gamma-ray fluxes for three Active Galactic Nuclei | |
| dc.type | text |