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Complex Physics in Cluster Cores: Showstopper for the Use of Clusters for Cosmology? | | Thomas H. Reiprich
; Daniel S. Hudson
; | | Date: |
16 Nov 2006 | | Abstract: | The influence of cool galaxy cluster cores on the X-ray luminosity--gravitational mass relation is studied with Chandra observations of 64 clusters in the HIFLUGCS sample. As preliminary results we find (i) a significant offset of cool core (CC) clusters to the high luminosity (or low mass) side compared to non-cool core (NCC) clusters, (ii) a smaller scatter of CC clusters compared to NCC clusters, (iii) a decreasing fraction of CC clusters with increasing cluster mass, (iv) a reduced scatter in the luminosity--mass relation for the entire sample if the luminosity is scaled properly with the central entropy. The implications of these results on the intrinsic scatter are discussed. | | Source: | arXiv, astro-ph/0611514 | | Services: | Forum | Review | PDF | Favorites | |
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