Non-thermal emission from relativistic cosmic ray (CR) electrons gives insight into the
strength and morphology of intra-cluster magnetic fields, as well as providing powerful …

Measuring the magnetic field in cosmic filaments reveals how the Universe is magnetized
and the process that magnetized it. Using the Rotation Measures (RM) at 144 MHz from the …

Many relaxed cool-core clusters host diffuse radio emission on scales of hundreds of
kiloparsecs: mini-haloes. However, the mechanism responsible for generating them, as well …

Context. Turbulence introduced into the intracluster medium (ICM) through cluster-merger
events transfers energy to non-thermal components, and can trigger the formation of diffuse …

The discovery of diffuse radio emission in galaxy clusters proved the existence of energetic
cosmic-ray electrons and cosmic magnetic fields on Mpc-scales in the Universe …

This is the first paper in a series of studies of the Coma cluster using the SRG/eROSITA X-
ray data obtained in the course of the calibration and performance verification observations …

Context. Abell 1033 is a merging galaxy cluster of moderate mass (M 500= 3.24× 10 14
M⊙). It hosts a broad variety of diffuse radio sources that are linked to different astrophysical …

We present the first detailed analysis of the radio halo in the merging galaxy cluster Abell
2256 using the LOw Frequency ARray, the upgraded Giant Metrewave Radio Telescope …

Context. Diffuse radio emission in galaxy clusters, namely radio halos and radio relics, is
usually associated with merger events. Despite the tremendous advances in observations in …

Context. Dynamical motions in the intra-cluster medium (ICM) can imprint distinctive features
on X-ray images that map the thermal bremsstrahlung emission from galaxy clusters, such …