The Evolution of Cluster Substructure

@article{Jeltema2004TheEO,
  title={The Evolution of Cluster Substructure},
  author={Tesla E. Jeltema and Claude R. Canizares and Mark W. Bautz and David A. Buote},
  journal={Astrophysics and space science library},
  year={2004},
  volume={301},
  pages={271-274}
}
Using Chandra archival data, we quantify the evolution of cluster morphology with redshift. To quantify cluster morphology, we use the power ratio method developed by Buote and Tsai (1995). Power ratios are constructed from moments of the two-dimensional gravitational potential and are, therefore, related to a cluster’s dynamical state. Our sample will include 40 clusters from the Chandra archive with redshifts between 0.11 and 0.89. These clusters were selected from two fairly complete flux… 

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