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20082026
most citedShock acceleration efficiency in radio relics

126 citations · 272 across the 13 of their papers we have counts for

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Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2026

A Brush with Turbulence: Probing the ICM Dynamics in the Merging Toothbrush Cluster using XRISM

Anjali Madangarli, Aurora Simionescu, Huub Röttgering +11

The Toothbrush Cluster (1RXS J0603.3+4214) is known for its northern radio relic, radio halo, and highly disturbed X-ray morphology. It shows features of both shock-driven and turb…

astro-ph.HE2024★ 5 cited

Jet interaction with galaxy cluster mergers

Paola Domínguez-Fernández, John ZuHone, Rainer Weinberger +4

AGN bubbles in cool-core galaxy clusters are believed to facilitate the transport of cosmic ray electrons (CRe) throughout the cluster. Recent radio observations are revealing comp…

astro-ph.HE2019★ 126 cited

Shock acceleration efficiency in radio relics

A. Botteon, G. Brunetti, D. Ryu +1

Radio relics in galaxy clusters are giant diffuse synchrotron sources powered in cluster outskirts by merger shocks. Although the relic-shock connection has been consolidated in re…

astro-ph.HE2011

Cosmic rays and diffuse non-thermal emission in galaxy clusters: an introduction

G. Brunetti

Recent multifrequency observations contribute to derive a comprehensive picture of the origin and evolution of relativistic particles in galaxy clusters. In this review I briefly d…

astro-ph.HE2009★ 15 cited

Constraining relativistic protons and magnetic fields in galaxy clusters through radio and gamma-ray observations : the case of A2256

G. Brunetti

Giant radio halos are the most relevant examples of diffuse synchrotron emission from galaxy clusters. A number of these sources have very steep spectrum, with spectral index $α\ge…