The Formation Histories of Galaxy Clusters
Abstract
Description
A sample of hundreds of simulated galaxy clusters is used to study the statistical properties of galaxy cluster formation. Individual assembly histories are discussed, the degree of virialization is demonstrated and various commonly used formation times are measured and inter-compared. In addition, the fraction of clusters which have ``recently'' undergone a major merger or significant mass jump is calculated as a function of lookback time and interval. The fraction of three- and four-body mergers is also studied.
24 pages, final version to appear in Astroparticle Physics
24 pages, final version to appear in Astroparticle Physics