Ultraluminous X-ray Sources, High Redshift QSOs and Active Galaxies
| dc.creator | Burbidge, G. | |
| dc.creator | Burbidge, E. M. | |
| dc.creator | Arp, H. C. | |
| dc.creator | Napier, W. M. | |
| dc.date | 2006-05-04 | |
| dc.date.accessioned | 2026-07-07T07:08:21Z | |
| dc.date.available | 2026-07-07T07:08:21Z | |
| dc.description | It is shown that all of the 32 point X-ray sources which lie within about 10' of the centre of nearby galaxies, and which have so far been optically identified are high redshift objects - AGN or QSOs. Thus the surface density of these QSOs p similar or equal to 0.1 per square arc minute. Some of them were originally discovered as X-ray sources and classified as ultraluminous X-ray sources (ULXs), nearly all of which lie near the centers of active galaxies. We demonstrate that this concentration around galactic nuclei is of high statistical significance: the probabiliy that p that they are accidental lies in the range one in a thousand to one in ten thousand, and apparently this excess cannot be accounted for by microlensing. | |
| dc.description | 6 pages, 2 figures, 1 table | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0605140 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0605140 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/110677 | |
| dc.subject | Astrophysics | |
| dc.title | Ultraluminous X-ray Sources, High Redshift QSOs and Active Galaxies | |
| dc.type | text |