activity
19962026
most citedTracing cosmic evolution with clusters of galaxies

863 citations · 8.8k across the 130 of their papers we have counts for

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Showing 2005Show all

6 papers · 1 filter

astro-ph2005★ 130 cited

A 70 kpc X-ray tail in the cluster A3627

M. Sun, C. Jones, W. Forman +3

We present the discovery of a 70 kpc X-ray tail behind the small late-type galaxy ESO137-001 in the nearby, hot (T=6.5 keV) merging cluster A3627, from both Chandra and XMM observa…

astro-ph2005★ 112 cited

Entropy Profiles in the Cores of Cooling Flow Clusters of Galaxies

Megan Donahue, Donald J. Horner, Kenneth W. Cavagnolo +1

The X-ray properties of a relaxed cluster of galaxies are determined primarily by its gravitational potential well and the entropy distribution of its intracluster gas. That entrop…

astro-ph2005★ 43 cited

An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters

Michael L. Balogh, Arif Babul, G. Mark Voit +4

(Abridged) We revisit the scaling relationships between the dark matter mass and observed X-ray luminosity and temperature of galaxy clusters and groups in the local Universe. Spec…

astro-ph2005★ 129 cited

An Observationally Motivated Framework for AGN Heating of Cluster Cores

G. Mark Voit, Megan Donahue

The cooling-flow problem is a long-standing puzzle that has received considerable recent attention, in part because the mechanism that quenches cooling flows in galaxy clusters is…

astro-ph2005★ 67 cited

Two Clusters with Radio-quiet Cooling Cores

Megan Donahue, G. Mark Voit, Christopher P. O'Dea +2

Radio lobes inflated by active galactic nuclei at the centers of clusters are a promising candidate for halting condensation in clusters with short central cooling times because th…

astro-ph2005★ 98 cited

Entropy amplification from energy feedback in simulated galaxy groups and clusters

S. Borgani, A. Finoguenov, S. T. Kay +4

We use hydrodynamical simulations of galaxy clusters and groups to study the effect of pre-heating on the entropy structure of the ICM. Our simulations account for non-gravitationa…