High Energy Emission from Galactic Black Hole Systems
| dc.creator | Goldwurm, A. | |
| dc.date | 2002-12-20 | |
| dc.date.accessioned | 2026-07-07T02:06:59Z | |
| dc.date.available | 2026-07-07T02:06:59Z | |
| dc.description | In the last decade our knowledge on galactic black hole systems and in particular on their high energy behavior has considerably improved. I will briefly review here the main results obtained by the high-energy missions SIGMA/GRANAT, Compton-GRO, Beppo-SAX and Rossi-XTE, on these objects and, in particular, I will discuss the spectral shapes observed at energies higher than 30 keV and the detections of high energy features at > 300 keV. Galactic black holes are indeed main targets for the ESA gamma-ray mission, INTEGRAL, to be launched in October 2002, and for the next gamma-ray missions SWIFT, AGILE and GLAST. We expect that a large amount of data will be collected in the next years and the perspectives for the high energy astrophysics of galactic black hole systems look very promising. | |
| dc.description | 9 pages, including 8 figures, submitted 15 July 2002, to appear in the proceedings of the XXII Moriond Astrophysics Meeting "The Gamma-Ray Universe" (March 9-16, 2002, Les Arcs, France), eds. A. Goldwurm, D. Neumann, and J. Tran Thanh Van, World Publisher (The Gioi), Hanoi (Vietnam) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0212502 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0212502 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5554 | |
| dc.subject | Astrophysics | |
| dc.title | High Energy Emission from Galactic Black Hole Systems | |
| dc.type | text |