activity
20082026
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 4.4k across the 69 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

17 papers · 1 filter

astro-ph.HE2024

A cooling flow around the low-redshift quasar H1821+643

H. R. Russell, P. E. J. Nulsen, A. C. Fabian +7

H1821+643 is the nearest quasar hosted by a galaxy cluster. The energy output by the quasar, in the form of intense radiation and radio jets, is captured by the surrounding hot atm…

astro-ph.HE2023★ 2 cited

Constraints on thermal conductivity in the merging cluster Abell 2146

A. Richard-Laferrière, H. R. Russell, A. C. Fabian +9

The cluster of galaxies Abell 2146 is undergoing a major merger and is an ideal cluster to study ICM physics, as it has a simple geometry with the merger axis in the plane of the s…

astro-ph.HE2023★ 12 cited

Chemical enrichment of the ICM within the Virgo cluster I: radial profiles

Efrain Gatuzz, J. Sanders, K. Dennerl +8

We present a detailed analysis of the elemental abundances distribution of the Virgo cluster using {\it XMM-Newton} observations. We included in the analysis a new EPIC-pn energy s…

astro-ph.HE2023★ 24 cited

AGN Feeding and Feedback in M84: From Kiloparsec Scales to the Bondi Radius

C. J. Bambic, H. R. Russell, C. S. Reynolds +3

We present the deepest Chandra observation to date of the galaxy M84 in the Virgo Cluster, with over 840 kiloseconds of data provided by legacy observations and a recent 730 kilose…

astro-ph.HE2022

The structure of cluster merger shocks: turbulent width and the electron heating timescale

H. R. Russell, P. E. J. Nulsen, D. Caprioli +10

We present a new 2 Ms Chandra observation of the cluster merger Abell 2146, which hosts two huge M~2 shock fronts each ~500 kpc across. For the first time, we resolve and measure t…

astro-ph.HE2022★ 14 cited

Turbulent magnetic fields in merging clusters: A case study of Abell 2146

Urmila Chadayammuri, John ZuHone, Paul Nulsen +2

Kelvin-Helmholtz Instabilities (KHI) along contact discontinuities in galaxy clusters have been used to constrain the strength of magnetic fields in galaxy clusters, following the…

astro-ph.HE2021★ 105 cited

New constraints on light Axion-Like Particles using Chandra Transmission Grating Spectroscopy of the powerful cluster-hosted quasar H1821+643

Júlia Sisk Reynés, James H. Matthews, Christopher S. Reynolds +3

Axion-Like Particles (ALPs) are predicted by several Beyond the Standard Model theories, in particular, string theory. In the presence of an external magnetic field perpendicular t…

astro-ph.HE2021★ 1 cited

Constraining Merging Galaxy Clusters with X-ray and Lensing Simulations and Observations: The case of Abell 2146

Urmila Chadayammuri, John ZuHone, Paul Nulsen +5

Galaxy cluster mergers are a powerful laboratory for testing cosmological and astrophysical models. However, interpreting individual merging clusters depends crucially on their mer…

astro-ph.HE2021★ 8 cited

Suppressed cooling and turbulent heating in the core of X-ray luminous clusters RXCJ1504.1-0248 and Abell 1664

Haonan Liu, Andrew C. Fabian, Ciro Pinto +3

We present the analysis of XMM-Newton observations of two X-ray luminous cool core clusters, RXCJ1504.1-0248 and Abell 1664. The Reflection Grating Spectrometer reveals a radiative…

astro-ph.HE2019★ 5 cited

The Advanced X-ray Imaging Satellite

Richard F. Mushotzky, James Aird, Amy J. Barger +41

Much of the baryonic matter in the Universe, including the most active and luminous sources, are best studied in the X-ray band. Key advances in X-ray optics and detectors have pav…

astro-ph.HE2019★ 21 cited

Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups

Haonan Liu, Ciro Pinto, Andrew C. Fabian +2

We present a spectral analysis of cool and cooling gas in 45 cool-core clusters and groups of galaxies obtained from Reflection Grating Spectrometer (RGS) XMM- observations…

astro-ph.HE2018★ 18 cited

AGN feedback in the Phoenix cluster

Ciro Pinto, Christopher J. Bambic, Jeremy S. Sanders +5

Active galactic nuclei (AGN) release a huge amount of energy into the intracluster medium (ICM) with the consequence of offsetting cooling and star formation (AGN feedback) in the…

astro-ph.HE2016★ 124 cited

Hitomi constraints on the 3.5 keV line in the Perseus galaxy cluster

Hitomi Collaboration, Felix A. Aharonian, Hiroki Akamatsu +215

High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E=3.5 keV emission line reported in several low-resolution studies of va…

astro-ph.HE2015★ 1 cited

Effects of the variability of the nucleus of NGC1275 on X-ray observations of the surrounding intracluster medium

A. C. Fabian, S. A. Walker, C. Pinto +2

The active galaxy NGC1275 lies at the centre of the Perseus cluster of galaxies, which is the X-ray brightest cluster in the Sky. The nucleus shows large variability over the past…

astro-ph.HE2014★ 24 cited

The X-ray spectrum of the cooling-flow quasar H1821+643 : A massive black hole feeding off the intracluster medium

Christopher S. Reynolds, Anne M. Lohfink, Arif Babul +4

We present a deep Suzaku observation of H1821+643, an extremely rare example of a powerful quasar hosted by the central massive galaxy of a rich cooling-core cluster of galaxies. I…

astro-ph.HE2014★ 37 cited

The effect of the quasar H1821+643 on the surrounding intracluster medium: revealing the underlying cooling flow

S. A. Walker, A. C. Fabian, H. R. Russell +1

We present a detailed study of the thermodynamic properties of the intracluster medium of the only low redshift galaxy cluster to contain a highly luminous quasar, H1821+643. The c…

astro-ph.HE2009★ 70 cited

The X-ray luminous cluster underlying the bright radio-quiet quasar H1821+643

H. R. Russell, A. C. Fabian, J. S. Sanders +4

We present a Chandra observation of the only low redshift, z=0.299, galaxy cluster to contain a highly luminous radio-quiet quasar, H1821+643. By simulating the quasar PSF, we subt…