TeV Gamma-Ray Astrophysics
| dc.creator | Ribo, M. | |
| dc.date | 2008-01-18 | |
| dc.date.accessioned | 2026-07-07T08:55:21Z | |
| dc.date.available | 2026-07-07T08:55:21Z | |
| dc.description | The window of TeV Gamma-Ray Astrophysics was opened less than two decades ago, when the Crab Nebula was detected for the first time. After several years of development, the technique used by imaging atmospheric Cherenkov telescopes like HESS, MAGIC or VERITAS, is now allowing to conduct sensitive observations in the TeV regime. Water Cherenkov instruments like Milagro are also providing the first results after years of integration time. Different types of extragalactic and galactic sources have been detected, showing a variety of interesting phenomena that are boosting theory in very high energy gamma-ray astrophysics. Here I review some of the most interesting results obtained up to now, making special emphasis in the field of X-ray/gamma-ray binaries. | |
| dc.description | Invited review at the Frascati Workshop 2007, Vulcano, Italy, May 28 - June 2 on "Multifrequency Behaviour of High Energy Cosmic Sources". ChJAA, in press. 12 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/0801.2906 | |
| dc.identifier | http://arxiv.org/abs/0801.2906 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/146242 | |
| dc.subject | Astrophysics | |
| dc.title | TeV Gamma-Ray Astrophysics | |
| dc.type | text |