activity
19952018
most citedStellar and total baryon mass fractions in groups and clusters since redshift 1

328 citations · 3.3k across the 69 of their papers we have counts for

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astro-ph2008★ 18 cited

Alignment of Galaxies and Clusters

Yasuhiro Hashimoto, J. Patrick Henry, Hans Boehringer

We investigated the influence of environment on cluster galaxies by examining the alignment of the brightest cluster galaxy (BCG) position angle with respect to the host cluster X-…

astro-ph2008★ 36 cited

Diffuse stellar emission in X-ray luminous galaxy clusters at z~0.3 I. Is the diffuse optical light boosted and rejuvenated in merging clusters?

D. Pierini, S. Zibetti, F. Braglia +4

[Abridged] We searched for diffuse stellar emission around BCGs in three of the most X-ray luminous clusters found at z~0.3 in the REFLEX cluster survey and observed with XMM-Newto…

astro-ph2008★ 14 cited

Indications for 3 Mpc-scale large-scale structure associated with an X-ray luminous cluster of galaxies at z=0.95

R. Fassbender, H. Boehringer, G. Lamer +5

X-ray luminous clusters of galaxies at z~1 are emerging as major cosmological probes and are fundamental tools to study the cosmic large-scale structure and environmental effects o…

astro-ph2008★ 222 cited

Searching for Cool Core Clusters at High redshift

Joana S. Santos, Piero Rosati, Paolo Tozzi +3

We investigate the detection of Cool Cores (CCs) in the distant galaxy cluster population, with the purpose of measuring the CC fraction out to redshift 0.7 < z < 1.4. Using a samp…

astro-ph2008★ 204 cited

Galaxy-cluster gas-density distributions of the Representative XMM-Newton Cluster Structure Survey (REXCESS)

J. H. Croston, G. W. Pratt, H. Boehringer +7

We present a study of the structural and scaling properties of the gas distributions in the intracluster medium (ICM) of 31 nearby (z < 0.2) clusters observed with XMM-Newton, whic…

astro-ph2007

Width of X-ray lines in cooling flows

P. Rebusco, E. Churazov, R. A. Sunyaev +2

The dissipation of turbulent gas motions is one of the likely mechanisms that has been proposed to heat the intracluster medium (ICM) in the cores of clusters and groups of galaxie…