Deep Sky Objects and the X-ray Background
| dc.creator | Fabian, A. C. | |
| dc.date | 2001-03-27 | |
| dc.date.accessioned | 2026-07-25T11:31:57Z | |
| dc.description | Deep observations of the X-ray Sky have now resolved most of the X-ray Background. Obscured active galaxies are a key component. The obscured objects which dominate at fluxes above $10^{-15}\ergpcmsqps$ are discussed and models in which the growth of wind-blowing active nuclei determine both black hole and galaxy mass are presented. The power from accretion is large and can easily influence the gas in a host galaxy, as well as heat the intergalactic medium. | |
| dc.description | 9 pages, 3 figures, To appear in Proc. of "X-ray astronomy 2000", (Palermo Sep. 2000), Eds. R. Giacconi, L. Stella, S. Serio, ASP Conf. Series, in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0103439 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0103439 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/3476 | |
| dc.subject | Astrophysics | |
| dc.title | Deep Sky Objects and the X-ray Background | |
| dc.type | text |