The nature of the soft X-ray emission in obscured AGN
| dc.creator | Bianchi, Stefano | |
| dc.creator | Guainazzi, Matteo | |
| dc.date | 2006-11-02 | |
| dc.date.accessioned | 2026-07-07T10:40:43Z | |
| dc.date.available | 2026-07-07T10:40:43Z | |
| dc.description | The origin of the soft X-ray emission in obscured AGN is still largely unknown. However, important progresses have been made thanks to the high energy and spatial resolution of XMM-Newton and Chandra. We review here the latest results on this issue, focusing on the physical properties of the material responsible for the soft X-ray emission and its relation to the circumnuclear environment, putting them in the general context of our understanding of the AGN structure and its feedback to the host galaxy. | |
| dc.description | 8 pages, 12 figures, invited review talk at the Workshop "The multicoloured landscape of compact objects and their explosive origin", Cefalu' (Sicily), 11-24 June 2006, to be published by AIP | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611045 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611045 | |
| dc.identifier | AIPConf.Proc.924:822-829,2007 | |
| dc.identifier | doi:10.1063/1.2774948 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/181414 | |
| dc.subject | Astrophysics | |
| dc.title | The nature of the soft X-ray emission in obscured AGN | |
| dc.type | text |