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20242026
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astro-ph.CO2026

MeerKAT observations of Abell 1775 and Abell 1795: the discovery of a hadronic radio halo?

R. J. van Weeren, E. Osinga, G. Brunetti +13

Giant radio haloes are diffuse synchrotron sources typically found in merging galaxy clusters, while smaller mini-haloes occur in cool-core clusters. Both trace cosmic-ray electron…

astro-ph.CO2025

Magnetic Fields in the Shapley Supercluster Core with POSSUM: Challenging Model Predictions

D. Alonso-López, S. P. O'Sullivan, A. Bonafede +18

Faraday Rotation Measure (RM) Grids provide a sensitive means to trace magnetized plasma across a wide range of cosmic environments. We study the RM signal from the Shapley Supercl…

astro-ph.CO2025

Discovery of Diffuse Radio Emission in a Massive z=1.709 Cool Core Cluster: A Candidate Radio Mini-Halo

Julie Hlavacek-Larrondo, Roland Timmerman, Christoph Pfrommer +10

Clusters of galaxies host spectacular diffuse radio sources, extending over scales from 100 kpc to several Mpcs. These sources, with extremely faint surface brightness (Jy/arcs…

astro-ph.CO2025

The phase-space of tailed radio galaxies in massive clusters

Stefan van der Jagt, Erik Osinga, Reinout J. van Weeren +4

The radio jets of radio galaxies in galaxy clusters are often bent due to the ram pressure of the intracluster medium. In this paper we start with a well-defined sample of galaxy c…

astro-ph.CO2025

Probing cluster magnetism with embedded and background radio sources in Planck clusters

Erik Osinga, Reinout J. van Weeren, Lawrence Rudnick +6

Magnetic fields remain an enigmatic part of the content of galaxy clusters. Faraday rotation and depolarisation of extragalactic radio sources are useful probes, but the limited av…

astro-ph.CO2024

Serendipitous decametre detection of ultra steep spectrum radio emission in Abell 655

C. Groeneveld, R. J. van Weeren, A. Botteon +5

Some galaxy clusters contain non-thermal synchrotron emitting plasma permeating the intracluster medium (ICM). The spectral properties of this radio emission are not well character…