activity
19952026
most citedHeating Hot Atmospheres with Active Galactic Nuclei

1.3k citations · 16.2k across the 255 of their papers we have counts for

collaborators

247 papers

astro-ph.GA2026

Cavity-driven Gas Transport in Cool-Core Clusters: Implications for Multiphase Gas Cooling

Prathamesh Tamhane, Brian McNamara, Paul Nulsen

We present a study of gas uplift by cavities and its role in promoting the formation of molecular gas in cool-core galaxy clusters. Using a sample of 24 clusters, we quantify the p…

astro-ph.HE2026

Gas Motions in Hydra-A: XRISM Constraints on ICM Kinematics Across Jet-Inflated Cavities

Anwesh Majumder, B. R. McNamara, P. E. J. Nulsen +8

We report on two deep XRISM observations of the central and northern regions of Hydra-A's X-ray atmosphere covering the bubbles inflated by jets from the central galaxy's active ga…

astro-ph.HE2026

Resolving the temporal evolution of M87 jet with -arcsec Chandra observations

Camille Poitras, Gerrit Schellenberger, Ralph Kraft +3

We present a 13-year Chandra/HRC-I study of the M87 jet, using point-spread-function deconvolution to achieve unprecedented sub-arcsecond X-ray resolution of its kiloparsec-scale s…

astro-ph.GA2026

DINGO/GAMA /WAVES: HI-halo mass relation

Ajay Dev, Martin Meyer, Simon P. Driver +17

We investigate the relation between neutral atomic hydrogen (HI) and dark matter halo mass (HIHM) using observations from the Deep Investigation of Neutral Gas Origins (DINGO) pilo…

astro-ph.HE2026

Are X-ray Atmospheres Heated by Turbulent Dissipation? XRISM Constraints

B. R. McNamara, A. C. Fabian, H. R. Russell +5

We evaluate whether dissipation of turbulence injected into hot cluster atmospheres by jets and bubbles can offset radiative cooling flows. No trends are found between atmospheric…

astro-ph.GA2026

The splash beneath the largest radio bubble in a cluster core

H. R. Russell, P. E. J. Nulsen, A. C. Fabian +3

We present a 100 ks XRISM Resolve observation of the Ophiuchus cluster that measures turbulence and bulk motion in the wake of the largest radio bubble on the sky. We detect a sign…