On the Simbol-X capability of detecting red/blue-shifted emission and absorption Fe K lines
| dc.creator | Tombesi, F. | |
| dc.creator | Cappi, M. | |
| dc.creator | Ponti, G. | |
| dc.creator | Malaguti, G. | |
| dc.creator | Palumbo, G. G. C. | |
| dc.date | 2007-12-20 | |
| dc.date.accessioned | 2026-07-07T08:50:37Z | |
| dc.date.available | 2026-07-07T08:50:37Z | |
| dc.description | The detection of red/blue-shifted iron lines in the spectra of astronomical X-ray sources is of great importance, as it allows to trace the environment around compact objects, like black holes in AGNs. We report on extensive simulations to test the Simbol-X capability of detecting such spectral features, focusing on the low energy detector (0.5-30 keV). | |
| dc.description | 2 pages, 2 figures, to appear in proceedings of "Simbol-X: the hard X-ray Universe in focus", held in Bologna (Italy), May 14-16, 2007 | |
| dc.identifier | https://arxiv.org/abs/0712.3427 | |
| dc.identifier | http://arxiv.org/abs/0712.3427 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/144660 | |
| dc.subject | Astrophysics | |
| dc.title | On the Simbol-X capability of detecting red/blue-shifted emission and absorption Fe K lines | |
| dc.type | text |