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astro-ph2000
Temperature Structure of Four Merging Clusters Obtained with Chandra
M. Markevitch, A. Vikhlinin, P. Mazzotta +1
We present preliminary Chandra results on z=0.2 clusters A665, A2163 and A2218, and a z=0.05 cluster A754. For A754, A665 and A2163, we have derived first high-resolution projected…
astro-ph2000
Evolution of the cluster X-ray luminosity function from the WARPS survey
L. R. Jones, H. Ebeling, C. Scharf +5
The evolution of the X-ray luminosity function of clusters of galaxies has been measured to z=0.85 using over 150 X-ray selected clusters found in the WARPS survey. We find no evid…