The Twofold Quasar-galaxy Connection
| dc.creator | Cavaliere, A. | |
| dc.creator | Vittorini, V. | |
| dc.date | 1997-12-22 | |
| dc.date.accessioned | 2026-07-07T02:25:39Z | |
| dc.date.available | 2026-07-07T02:25:39Z | |
| dc.description | The rise and the fall of the QS population are explained in terms of massive black holes forming/accreting during the assemblage of the host galaxies, and of accretion rekindled by interactions of the host with companions in a group. We compute the LFs out to z= 6. We also predict the masses of relict black holes to be found in many galaxies. We compare the histories of the QSO and of the star light. | |
| dc.description | 4 pages, Latex, uses sprocl.sty, 1 ps-figure. Talk presented at the 12th Potsdam Cosmology Workshop in Sept. 1997, to appear in ``Large Scale Structures: Tracks and Traces'', eds. V. Mueller et al., World Scientific 1998 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9712295 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9712295 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11958 | |
| dc.subject | Astrophysics | |
| dc.title | The Twofold Quasar-galaxy Connection | |
| dc.type | text |