Semi-analytic galaxy formation: understanding the high redshift universe
| dc.creator | Baugh, C. M. | |
| dc.creator | Benson, A. J. | |
| dc.creator | Cole, S. | |
| dc.creator | Frenk, C. S. | |
| dc.creator | Lacey, C. G. | |
| dc.date | 2001-03-10 | |
| dc.date.accessioned | 2026-07-07T01:57:55Z | |
| dc.date.available | 2026-07-07T01:57:55Z | |
| dc.description | There is now compelling evidence in favour of the hierarchical structure formation paradigm. Semi-analytic modelling is a powerful tool which allows the formation and evolution of galaxies to be followed in a hierarchical framework. We review some of the latest developments in this area before discussing how such models can help us to interpret observations of the high redshift Universe. | |
| dc.description | 10 pages. Invited review to appear in the proceedings of the workshop on "QSO hosts and their environments", IAA, Granada, 10-12 Jan 2001 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0103156 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0103156 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2576 | |
| dc.subject | Astrophysics | |
| dc.title | Semi-analytic galaxy formation: understanding the high redshift universe | |
| dc.type | text |