Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

We review current understanding of the population of radio galaxies and radio-loud quasars
from an observational perspective, focusing on their large-scale structures and dynamics …

Context. During their lifetimes, galaxy clusters grow through the accretion of matter from the
filaments of the large-scale structure and from mergers with other clusters. These mergers …

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 …

We have performed magnetohydrodynamic (MHD) simulations of relativistic jets from
supermassive blackholes over a few tens of kpc for a range of jet parameters. One of the …

When astrophysical jets were discovered one hundred years ago, the field of numerical
simulations did not yet exit. Since the arrival of programmable computers though, numerical …

Young massive star clusters inhabit regions of star formation and play an essential role in
the galactic evolution. They are sources of both thermal and non-thermal radiation, and are …

We review numerical methods for simulations of cosmic ray (CR) propagation on galactic
and larger scales. We present the development of algorithms designed for …

Core-collapse supernova remnants are structures of the interstellar medium (ISM) left
behind the explosive death of most massive stars (). Since they result in the expansion of the …

High-resolution radio observations of cluster radio relics often show complex spatial and
spectral features. However, it is not clear what these features reveal about the underlying …