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19952023
most citedChandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation

1.4k citations · 21.5k across the 256 of their papers we have counts for

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Showing 2017 · astro-ph.HEShow all

5 papers · 2 filters

astro-ph.HE2017★ 49 cited

Gas sloshing regulates and records the evolution of the Fornax Cluster

Yuanyuan Su, Paul E. J. Nulsen, Ralph P. Kraft +7

We present results of a joint {\sl Chandra} and {\sl XMM-Newton} analysis of the Fornax Cluster, the nearest galaxy cluster in the southern sky. Signatures of merger-induced gas sl…

astro-ph.HE2017★ 19 cited

Probing the hot X-ray gas in the narrow-line region of Mrk 3

Akos Bogdan, Ralph P. Kraft, Daniel A. Evans +2

We study the prototypical Seyfert 2 galaxy, Markarian 3, based on imaging and high-resolution spectroscopy observations taken by the Chandra X-ray Observatory. We construct a decon…

astro-ph.HE2017★ 23 cited

Stripped elliptical galaxies as probes of ICM physics: III. Deep Chandra Observation of NGC 4552 - Measuring the Viscosity of the Intracluster Medium

Ralph Kraft, Elke Roediger, Marie Machacek +7

We present results from a deep (200 ks) Chandra observation of the early-type galaxy NGC 4552 (M89) which is falling into the Virgo cluster. Previous shallower X-ray observations o…

astro-ph.HE2017★ 28 cited

Buoyant AGN bubbles in the quasi-isothermal potential of NGC 1399

Yuanyuan Su, Paul E. J. Nulsen, Ralph P. Kraft +5

The Fornax Cluster is a low-mass cool-core galaxy cluster. We present a deep {\sl Chandra} study of NGC 1399, the central dominant elliptical galaxy of Fornax. The cluster center h…

astro-ph.HE2017★ 203 cited

The Case for Electron Re-Acceleration at Galaxy Cluster Shocks

Reinout J. van Weeren, Felipe Andrade-Santos, William A. Dawson +16

On the largest scales, the Universe consists of voids and filaments making up the cosmic web. Galaxy clusters are located at the knots in this web, at the intersection of filaments…