The Evolution of Structure in X-ray Clusters of Galaxies

Using Chandra archival data, we quantify the evolution of cluster morphology with redshift. Clusters form and grow through mergers with other clusters and groups, and the amount of substructure in clusters in the present epoch and how quickly it evolves with redshift depend on the underlying cosmolo...

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Bibliographic Details
Main Authors: Jeltema, Tesla E. (Contributor), Canizares, Claude R. (Contributor), Buote, David A. (Author), Bautz, Marshall W. (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Bautz, Mark W. (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2012-07-31T17:34:37Z.
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