Evolution of a correlation function of QSOs and the initial power spectrum of density fluctuations
| dc.creator | Chornij, Yu. | |
| dc.creator | Novosyadlyj, B. | |
| dc.date | 1999-11-22 | |
| dc.date.accessioned | 2026-07-07T02:34:35Z | |
| dc.date.available | 2026-07-07T02:34:35Z | |
| dc.description | The evolution of two-point space correlation function of QSOs is analyzed in the framework of the theory of the large scale structure formation. For given cosmological models the agreement between theoretical predictions and observational data on correlation function of QSOs is achieved by determination of scales of structures R(z), in which could be formed quasars at different redshifts z. It is shown that quasars could be formed in the nucleus of massive galaxies or groups of galaxies owing to merges at their central region. It depends on an amplitude of the power spectrum of the initial matter density fluctuations at galaxy-cluster scales. | |
| dc.description | 4 pages, 3 figers (Proceedings of Gamow Memorial International Conference "The Universe of Gamow: Origional Ideas in Astrophysics and Cosmology", Odessa, August 16-22, 1999; to be published in "Odessa Astron. Publ.", v.12, 1999) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9911411 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9911411 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15302 | |
| dc.subject | Astrophysics | |
| dc.title | Evolution of a correlation function of QSOs and the initial power spectrum of density fluctuations | |
| dc.type | text |