In a growing number of galaxy clusters diffuse extended radio sources have been found.
These sources are not directly associated with individual cluster galaxies. The radio …

Radio observations prove the existence of relativistic particles and magnetic field associated
with the intra-cluster-medium (ICM) through the presence of extended synchrotron emission …

We introduce the IllustrisTNG project, a new suite of cosmological magnetohydrodynamical
simulations performed with the moving-mesh code arepo employing an updated Illustris …

Diffuse cluster radio sources, in the form of radio halos and relics, reveal the presence of
cosmic rays and magnetic fields in the intracluster medium (ICM). These cosmic rays are …

On the largest scales, the Universe consists of voids and filaments making up the cosmic
web. Galaxy clusters are located at the knots in this web, at the intersection of filaments …

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

This book summarizes the science to be carried out by the upcoming Cherenkov Telescope
Array, a major ground-based gamma-ray observatory that will be constructed over the next …

Radio relics are the manifestation of electrons presumably being shock (re-) accelerated to
high energies in the outskirts of galaxy clusters. However, estimates of the shocks' strength …

The origin of extragalactic magnetic fields is still poorly understood. Based on a dedicated
suite of cosmological magneto-hydrodynamical simulations with the ENZO code we have …

Names: CTA Consortium (Organization) Title: Science with the Cherenkov Telescope
Array/by The CTA Consortium. Description: New Jersey: World Scientific, 2018.| Includes …