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X-ray temperature and morphology of z>0.8 clusters of galaxies

B. Holden·S. A. Stanford·P. Rosati·P. Tozzi·G. Squires·S. Borgani·P. Eisenhardt
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Abstract

We discuss our current progress in studying a sample of z>0.8 clusters of galaxies from the ROSAT Distant Cluster Survey. To date, we have Chandra observations for four of the ten clusters. We find that the morphology of two of these four are quite regular, with deviations from circular of less than 5%, while two are strikingly elliptical. When the temperatures and luminosities of our sample are grouped with six other high-redshift measurements, there is no measured evolution in the luminosity-temperature relation. We identify a number of X-ray emitting point sources that are potential cluster members. These could be sources of intracluster medium heating, adding the entropy necessary to explain the cluster luminosity-temperature relation.

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B. Holden, S. A. Stanford, P. Rosati, P. Tozzi, G. Squires, S. Borgani, P. Eisenhardt. 2001-10-01. X-ray temperature and morphology of z>0.8 clusters of galaxies. https://arxiv.org/abs/astro-ph/0110032

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