Thin synchrotron-emitting filaments are increasingly seen in the intracluster medium (ICM).
We present the first example of a direct interaction between a magnetic filament, a radio jet …

Abell 3266 is a massive and complex merging galaxy cluster that exhibits significant
substructure. We present new, highly sensitive radio continuum observations of Abell 3266 …

Diffuse radio emission has been detected in a considerable number of galaxy clusters and
groups, revealing the presence of pervasive cosmic magnetic fields, and of relativistic …

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 …

We simulate the evolution of relativistic eletrons injected into the medium of a small galaxy
cluster by a central radio galaxy, studying how the initial jet power affects the dispersal and …

Using a MeerKAT observation of the galaxy cluster A3562 (a member of the Shapley
supercluster), we have discovered a narrow, long and straight, very faint radio filament …

We report on the detection of diffuse radio emission with peculiar morphology in the central
region of the galaxy cluster Abell 2657. The most striking feature identified in our 144 MHz …

We present a new end-to-end pipeline for M ock O bservations of X-ray H aloes and A
nalysis (moxha) for hydrodynamic simulations of massive haloes, and use it to investigate X …

We simulate the evolution of relativistic electrons injected into the intracluster medium by five
radio galaxies. We study the spatial transport and the emission properties of the injected …

Context. Radio observations of galaxy clusters reveal a plethora of diffuse, steep-spectrum
sources related to the re-acceleration of cosmic-ray electrons, such as halos, relics, and …