Modeling the Clustering of Objects
| dc.creator | Salvador-Sole, E. | |
| dc.date | 1995-12-07 | |
| dc.date.accessioned | 2026-07-07T02:20:33Z | |
| dc.date.available | 2026-07-07T02:20:33Z | |
| dc.description | I review the main steps made so far towards the construction of a (semi) analytical model for describing the growth history of bound virialized objects or haloes in the gravitational instability scenario. I mainly focus on those models relying on the spherical collapse approximation which have led to the most complete description. I insist on the different assumptions of each model and outline their main advantages and shortcomings. The work is divided in two parts: a first one dealing with the theoretical mass function of objects, and a second one dealing with the typical growth times and rates. Particular attention is paid to a new model making the practical distinction between accretion and merger events. | |
| dc.description | 12 pages, uuencoded compressed latex file + 1 eps figure, to appear in the ASP conference series | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9512037 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9512037 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10244 | |
| dc.subject | Astrophysics | |
| dc.title | Modeling the Clustering of Objects | |
| dc.type | text |