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 …

There is a broad consensus that accretion onto supermassive black holes and consequent
jet formation power the observed emission from active galactic nuclei (AGNs). However …

We implement a black hole spin evolution and jet feedback model into SWIFT, a smoothed
particle hydrodynamics code. The jet power is determined self-consistently assuming that …

Energy deposition by active galactic nuclei jets into the ambient medium can affect galaxy
formation and evolution, the cooling of gas flows at the centres of galaxy clusters, and the …

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 …

We present THC: a new high-order flux-vector-splitting code for Newtonian and special-
relativistic hydrodynamics designed for direct numerical simulations of turbulent flows. Our …

Radio jets and the lobes they inflate are common in cool-core clusters and are known to play
a critical role in regulating the heating and cooling of the intracluster medium (ICM). This is …

Feedback processes by active galactic nuclei in the centres of galaxy clusters appear to
prevent large-scale cooling flows and impede star formation. However, the detailed heating …

Supermassive black hole binaries may be detectable by an upcoming suite of gravitational
wave experiments. Their binary nature can also be revealed by radio jets via a short-period …

Relativistic jets in active galactic nuclei (AGN) convert as much as half of their energy into
radiation. To explore the poorly understood processes that are responsible for this …