| HAL : in2p3-00368774, version 1 |
| Code Bibliographique ADS : 2008AIPC.1085..135G |
| DOI : 10.1063/1.3076629 |
| Fiche détaillée | Récupérer au format |
|
|
| 4th International Meeting on High Energy Gamma-Ray Astronomy, Heidelberg : Germany (2008) |
|
|
|
|
| A Multiwavelength View of High-Energy Processes in the Galactic Center Region |
|
|
| A. Goldwurm1, 2 |
|
|
| (12/2008) |
|
|
| The central 600 parsecs of our Galaxy can be considered a kind of laboratory for modern astrophysics because in the few square degrees of sky covered by this region, several important non-thermal high energy processes take place and can be studied in detail with the new telescopes operating both in on-ground and in space. In addition to the closest supermassive Black Hole to the solar system the region hosts several other compact and diffuse sources of high-energy radiation whose characteristics need to be studied at different wavelengths from radio to TeV gamma-rays in order to understand the physical processes at work. This paper presents a review of the characteristics of the Galactic Center region from a multiwavelength phenomenological point of view, and giving special emphasis to the sources and processes that shed ligth on the high-energy phenomena taking place in the region. |
|
|
|
|
|
|
|
|
|
|
| 1 : | APC - AstroParticule et Cosmologie |
| 2 : | IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers (ex DAPNIA) |
|
|
|
|
|
|
|
|
| APC - AHE |
|
|
|
|
| Thème(s) | : | Physique/Astrophysique/Phénomènes cosmiques de haute energie Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie |
|
|
| Galactic centre – galaxies – black holes |
| in2p3-00368774, version 1 | |
| http://hal.in2p3.fr/in2p3-00368774 | |
| oai:hal.in2p3.fr:in2p3-00368774 | |
| Contributeur : Simone Lantz | |
| Soumis le : Mardi 17 Mars 2009, 15:46:18 | |
| Dernière modification le : Samedi 23 Juin 2012, 12:58:43 | |