X-Ray Emission in Gamma-Ray Blazars
| dc.creator | Ghisellini, Gabriele | |
| dc.date | 1996-12-04 | |
| dc.date.accessioned | 2026-07-07T02:22:27Z | |
| dc.date.available | 2026-07-07T02:22:27Z | |
| dc.description | Although the gamma-ray emission in blazars dominates the power output, there are crucial informations carried by the X-rays. Indeed, their paucity, together with the short variability timescales observed both at X and gamma-ray energies constrains the location, along the jet, of the active region responsible for most of the emission. Furthermore, the knowledge of the X-ray flux and spectrum helps in defining the overall spectral energy distribution (SED) of blazars, allowing to discriminate between models. | |
| dc.description | 4 pages, 2 figures, to be published in the Proceedings of the conference "Gamma-ray emitting AGN", Heidelberg, October 16-18 1996, eds. J. Kirk and S. Wagner | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9612042 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9612042 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10883 | |
| dc.subject | Astrophysics | |
| dc.title | X-Ray Emission in Gamma-Ray Blazars | |
| dc.type | text |