Journal
ASTROPARTICLE PHYSICS
Volume 24, Issue 4-5, Pages 316-333Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.astropartphys.2005.07.006
Keywords
cosmology; galaxy clusters; mergers; formation times
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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. (c) 2005 Elsevier B.V. All rights reserved.
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