activity
20192025
most citedFast magnetic field amplification in distant galaxyclusters

64 citations · 379 across the 10 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2025

Resurging from the ashes: A spectral study of seven candidate revived radio fossils in nearby low-mass galaxy clusters

L. Bruno, A. Botteon, D. Dallacasa +17

Complex energy transfer processes in the intracluster medium (ICM) can revive fossil (with spectral ages Myr) plasma initially generated by radio galaxies. This leads to t…

astro-ph.HE2025

Discovery of large-scale radio emission enveloping the mini-halo in the most X-ray luminous galaxy cluster RX~J1347.5-1145

D. N. Hoang, M. Brüggen, A. Bonafede +8

Diffuse radio sources, known as mini-halos and halos, are detected at the centres of galaxy clusters. These centralized diffuse sources are typically observed individually, with bo…

astro-ph.CO202254 cited

Magnetic fields and relativistic electrons fill entire galaxy cluster

A. Botteon, R. J. van Weeren, G. Brunetti +12

The hot plasma within merging galaxy clusters is predicted to be filled with shocks and turbulence that may convert part of their kinetic energy into relativistic electrons and mag…

astro-ph.CO202119 cited

Discovery of a radio halo (and relic) in a M cluster

A. Botteon, R. Cassano, R. J. van Weeren +12

Radio halos are diffuse synchrotron sources observed in dynamically unrelaxed galaxy clusters. Current observations and models suggest that halos trace turbulent regions in the int…

astro-ph.CO2021

The LOFAR and JVLA view of the distant steep spectrum radio halo in MACS J1149.5+2223

L. Bruno, K. Rajpurohit, G. Brunetti +11

Radio halos and relics are Mpc-scale diffuse radio sources in galaxy clusters, with a steep spectral index (). It has been proposed that they arise from part…

astro-ph.GA202131 cited

Downstream depolarization in the Sausage relic: a 1-4 GHz Very Large Array study

G. Di Gennaro, R. J. van Weeren, L. Rudnick +10

Radio relics are elongated sources related to shocks driven by galaxy cluster merger events. Although these objects are highly polarized at GHz frequencies (), high-r…