activity
19952004
most citedChandra temperature profiles for a sample of nearby relaxed galaxy clusters

527 citations · 535 across the 5 of their papers we have counts for

collaborators
Showing astro-phShow all

18 papers · 1 filter

astro-ph200723 cited

On the width of cold fronts in clusters of galaxies due to conduction

F. Xiang, E. Churazov, K. Dolag +2

We consider the impact of thermal conduction in clusters of galaxies on the (unmagnetized) interface between a cold gaseous cloud and a hotter gas flowing over the cloud (the so-ca…

astro-ph2007260 cited

The Representative XMM-Newton Cluster Structure Survey (REXCESS) of an X-ray Luminosity Selected Galaxy Cluster Sample

H. Boehringer, P. Schuecker, G. W. Pratt +31

The largest uncertainty for cosmological studies using clusters of galaxies is introduced by our limited knowledge of the statistics of galaxy cluster structure, and of the scaling…

astro-ph2007755 cited

Shocks and cold fronts in galaxy clusters

Maxim Markevitch, Alexey Vikhlinin

Table of contents (abridged): COLD FRONTS Origin and evolution of merger cold fronts Cold fronts in cluster cool cores . . . Simulations of gas sloshing. Origin of density disconti…

astro-ph2004527 cited

Chandra temperature profiles for a sample of nearby relaxed galaxy clusters

A. Vikhlinin, M. Markevitch, S. S. Murray +3

We present Chandra gas temperature profiles at large radii for a sample of 13 nearby, relaxed galaxy clusters and groups, which includes A133, A262, A383, A478, A907, A1413, A1795,…

astro-ph2003

The 160 Square Degree ROSAT Survey - Revised Catalog & Cluster Evolution

Christopher Mullis, Brian McNamara, Hernan Quintana +6

We have constructed a large, statistically complete sample of galaxy clusters serendipitously detected as extended X-ray sources in 647 ROSAT PSPC pointed observations. The survey…

astro-ph20032 cited

A High Angular Resolution View of Hot Gas in Clusters, Groups, and Galaxies

W. Forman, E. Churazov, L. David +6

We discuss two themes from Chandra and XMM-Newton observations of galaxies, groups, and clusters. First, we review observational aspects of cluster formation and evolution as matte…