Mathematics – Logic
Scientific paper
Aug 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011scgg.conf...25j&link_type=abstract
"Structure in Clusters and Groups of Galaxies in the Chandra Era, 2011 Chandra Science Workshop held July 12-14, 2011. Edited by
Mathematics
Logic
Scientific paper
In this talk I will present a flux limited sample of galaxy clusters observed with Chandra which exhibit sloshing gas in their cores. This work confirms that sloshing is indeed common in cool core clusters, as it should be based on the persistence of the resulting morphology and the frequency of interactions which may initiate it. With a particular emphasis on comparing the morphological traits of the sloshing gas with those predicted by simulations, I will describe how gas sloshing may be used to constrain the merger histories of galaxy clusters on an individual basis, as well as constrain the build up of structure over cosmic times.
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