The X-ray properties of luminous infrared galaxies and their contribution to the X-ray background
| dc.creator | Risaliti, G. | |
| dc.date | 2000-01-21 | |
| dc.date.accessioned | 2026-07-07T01:51:50Z | |
| dc.date.available | 2026-07-07T01:51:50Z | |
| dc.description | We present a study of a sample of luminous infrared galaxies (LIGs, L_IR > 10^11 L_sun) observed in the hard (2-10 keV) X rays. The main results are: 1) most LIGs are powered both by AGN and starburst activity; 2) the AGNs in our sample are absorbed in the infrared by a lower N_H than in the X rays or, alternatively, the dust-to-gas ratio is lower than galactic; 3) the study of a subsample of sources observed in the 20-200 keV band indicates that most of the AGNs hosted by the LIGs are heavily obscured up to 100 keV and, therefore, their contribution to the X-ray background must be small. | |
| dc.description | To appear in the proceedings of the conference "Large Scale Structure in the X-ray Universe", Santorini, Greece, September 1999, 4 pages, 2 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0001375 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0001375 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/426 | |
| dc.subject | Astrophysics | |
| dc.title | The X-ray properties of luminous infrared galaxies and their contribution to the X-ray background | |
| dc.type | text |