Statistical analysis of the X-ray morphology of galaxy clusters
The morphological analysis of galaxy clusters in X-rays allows a reliable determination of their dynamical state. Substructures on (sub-)Mpc scale influence the gravitational potential of a cluster and manifest themselves in the X-ray surface brightness distribution as secondary peaks or overall irr...
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Ludwig-Maximilians-Universität München
2013
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| Online Access: | http://edoc.ub.uni-muenchen.de/16520/1/Weissmann_Alexandra.pdf http://nbn-resolving.de/urn:nbn:de:bvb:19-165203 |