activity
20152025
most citedCooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters

199 citations · 320 across the 11 of their papers we have counts for

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Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2025

XMAGNET : Kinetic, Thermal and Magnetic AGN Feedback in Massive Galaxies at Halo Masses M

Deovrat Prasad, Philipp Grete, Brian O'Shea +5

The interplay between radiative cooling of the circumgalactic medium (CGM) and feedback heating governs the evolution of the universe's most massive galaxies. This paper presents s…

astro-ph.GA2025

Precipitation plausible: magnetized thermal instability in the intracluster medium

Benjamin D. Wibking, G. Mark Voit, Brian W. O'Shea

Observations of galaxy-cluster cores reveal that AGN feedback is strongly associated with both a short central cooling time () and accumulation…

astro-ph.GA2025★ 5 cited

XMAGNET: Velocity structure functions of active galactic nucleus-driven turbulence in the multiphase intracluster medium

M. Fournier, P. Grete, M. Brüggen +5

Significant theoretical and observational efforts are underway to investigate the properties of turbulence in the hot plasma that pervades galaxy clusters. Spectroscopy has been us…

astro-ph.GA2025★ 1 cited

The XMAGNET exascale MHD simulations of SMBH feedback in galaxy groups and clusters: Overview and preliminary cluster results

Philipp Grete, Brian W. O'Shea, Forrest W. Glines +5

We present initial results from extremely well-resolved 3D magnetohydrodynamical simulations of idealized galaxy clusters, conducted using the AthenaPK code on the Frontier exascal…

astro-ph.GA2024

Precipitation possible: turbulence-driven thermal instability with constrained entropy profiles

Benjamin D. Wibking, G. Mark Voit, Brian W. O'Shea

Precipitation of cold gas due to thermal instability in both galaxy clusters and the circumgalactic medium may regulate AGN feedback. We investigate thermal instability in idealize…

astro-ph.GA2024★ 15 cited

The properties of magnetised cold filaments in a cool-core galaxy cluster

Martin Fournier, Philipp Grete, Marcus Brüggen +2

Filaments of cold gas ( K) are found in the inner regions of many cool-core clusters. These structures are thought to play a major role in the regulation of feedback…

astro-ph.GA2023★ 3 cited

The Case for Hot-Mode Accretion in Abell 2029

Deovrat Prasad, G. Mark Voit, Brian W. O'Shea

Radiative cooling and AGN heating are thought to form a feedback loop that regulates the evolution of low redshift cool-core galaxy clusters. Numerical simulations suggest that for…

astro-ph.GA2020★ 34 cited

A Black-Hole Feedback Valve in Massive Galaxies

G. M. Voit, G. L. Bryan, D. Prasad +6

Star formation in the universe's most massive galaxies proceeds furiously early in time but then nearly ceases. Plenty of hot gas remains available but does not cool and condense i…

astro-ph.GA2019

Circumgalactic Gas and the Precipitation Limit

G. M. Voit, A. Babul, Iu. Babyk +15

During the last decade, numerous and varied observations, along with increasingly sophisticated numerical simulations, have awakened astronomers to the central role the circumgalac…

astro-ph.GA2016★ 63 cited

Triggering and Delivery Algorithms for AGN Feedback

Gregory R. Meece, G. Mark Voit, Brian W. O'Shea

We compare several common sub-grid implementations of AGN feedback, focusing on the effects of different triggering mechanisms and the differences between thermal and kinetic feedb…

astro-ph.GA2015★ 199 cited

Cooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters

Yuan Li, Greg L. Bryan, Mateusz Ruszkowski +3

Numerical simulations of active galactic nuclei (AGN) feedback in cool-core galaxy clusters have successfully avoided classical cooling flows, but often produce too much cold gas.…