X-ray and soft gamma-ray behaviour of the Galactic source 1E 1743.1-2843
| dc.creator | Del Santo, M. | |
| dc.creator | Sidoli, L. | |
| dc.creator | Bazzano, A. | |
| dc.creator | Cocchi, M. | |
| dc.creator | De Cesare, G. | |
| dc.creator | Paizis, A. | |
| dc.creator | Ubertini, P. | |
| dc.date | 2005-11-10 | |
| dc.date.accessioned | 2026-07-07T06:44:59Z | |
| dc.date.available | 2026-07-07T06:44:59Z | |
| dc.description | The X-ray persistent source 1E 1743.1-2843, located in the Galactic Centre region, has been detected by all X-ray telescope above 2 keV, whereas it is not visible in the soft X-rays (i. e. Rosat) because of the high column density along the line-of-sight. Moreover, the nature of this source remains still unknown. The gamma-ray satellite INTEGRAL has long observed the Galactic Centre region in the framework of the Core Programme. We report on results of two years of INTEGRAL observations of 1E 1743.1--2843 detected for the first time in the soft gamma-ray band. Since the source does not show any evidence for strong variability, we present the broad-band spectral analysis using not simultaneous XMM-Newton observations. | |
| dc.description | 2 pages, 2 figures, to appear in the proceedings of "The X-ray Universe 2005", San Lorenzo de El Escorial (Spain), 26-30 September 2005 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0511301 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0511301 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/102935 | |
| dc.subject | Astrophysics | |
| dc.title | X-ray and soft gamma-ray behaviour of the Galactic source 1E 1743.1-2843 | |
| dc.type | text |