activity
19982022
most citedA very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction

650 citations · 5.6k across the 49 of their papers we have counts for

collaborators

51 papers

astro-ph.GA2022★ 16 cited

Radio jet-ISM interaction and positive radio-mechanical feedback in Abell 1795

Prathamesh D. Tamhane, Brian R. McNamara, Helen R. Russell +8

We present XSHOOTER observations with previous ALMA, MUSE and observations to study the nature of radio-jet triggered star formation and the interaction of radio jets with th…

astro-ph.HE2016★ 29 cited

Insights into the location and dynamics of the coolest X-ray emitting gas in clusters of galaxies

Ciro Pinto, Andrew C. Fabian, Anna Ogorzalek +10

We extend our previous study of the cool gas responsible for the emission of OVII X-ray lines in the cores of clusters and groups of galaxies. This is the coolest X-ray emitting ph…

astro-ph.GA2016★ 38 cited

HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster

A. C. Fabian, S. A. Walker, H. R. Russell +14

Narrow-band HST imaging has resolved the detailed internal structure of the 10 kpc diameter H alpha+[NII] emission line nebulosity in NGC4696, the central galaxy in the nearby Cent…

astro-ph.CO2015★ 20 cited

Dynamical analysis of galaxy cluster merger Abell 2146

J. A. White, R. E. A. Canning, L. J. King +12

We present a dynamical analysis of the merging galaxy cluster system Abell 2146 using spectroscopy obtained with the Gemini Multi-Object Spectrograph on the Gemini North telescope.…

astro-ph.GA2015★ 12 cited

Collisional excitation of [C II], [O I] and CO in Massive Galaxies

R. E. A. Canning, G. J. Ferland, A. C. Fabian +5

Many massive galaxies at the centres of relaxed galaxy clusters and groups have vast reservoirs of cool (~10,000 K) and cold (~100 K) gas. In many low redshift brightest group and…

astro-ph.GA2014★ 16 cited

Implications of Coronal Line Emission in NGC 4696

M. Chatzikos, R. J. R. Williams, G. J. Ferland +7

We announce a new facility in the spectral code CLOUDY that enables tracking the evolution of a cooling parcel of gas with time. For gas cooling from temperatures relevant to galax…