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20052026
most citedTurbulent Heating in Galaxy Clusters Brightest in X-rays

340 citations · 1.8k across the 33 of their papers we have counts for

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Showing astro-ph.COShow all

12 papers · 1 filter

astro-ph.CO2018★ 14 cited

Revealing a Highly-Dynamic Cluster Core in Abell 1664 with Chandra

Michael S. Calzadilla, Helen R. Russell, Michael McDonald +11

We present new, deep (245 ks) Chandra observations of the galaxy cluster Abell 1664 (). These images reveal rich structure, including elongation and accompanying compre…

astro-ph.CO2018★ 17 cited

Discovery of a diffuse optical line emitting halo in the core of the Centaurus cluster of galaxies: Line emission outside the protection of the filaments

S. L. Hamer, A. C. Fabian, H. R. Russell +6

We present the discovery of diffuse optical line emission in the Centaurus cluster seen with the MUSE IFU. The unparalleled sensitivity of MUSE allows us to detect the faint emissi…

astro-ph.CO2014★ 27 cited

The bow shock, cold fronts and disintegrating cool core in the merging galaxy group RXJ0751.3+5012

H. R. Russell, A. C. Fabian, B. R. McNamara +6

We present a new Chandra X-ray observation of the off-axis galaxy group merger RXJ0751.3+5012. The hot atmospheres of the two colliding groups appear highly distorted by the merger…

astro-ph.CO2013★ 54 cited

Cold gas dynamics in Hydra-A: evidence for a rotating disk

S. L. Hamer, A. C. Edge, A. M. Swinbank +15

We present multi-frequency observations of the radio galaxy Hydra-A (3C218) located in the core of a massive, X-ray luminous galaxy cluster. IFU spectroscopy is used to trace the k…

astro-ph.CO2013★ 157 cited

The origin of cold gas in giant elliptical galaxies and its role in fueling radio-mode AGN feedback

N. Werner, J. B. R. Oonk, M. Sun +12

We present a multi-wavelength study of the interstellar medium in eight nearby, X-ray and optically bright, giant elliptical galaxies. Using Herschel PACS, we map the cold gas in t…

astro-ph.CO2013★ 44 cited

Linear Structures in the Core of the Coma Cluster of Galaxies

J. S. Sanders, A. C. Fabian, E. Churazov +4

The hot X-ray emitting plasma in galaxy clusters is predicted to have turbulent motions which can contribute around ten percent of the cluster's central energy density. We report d…