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 …

Analytical models describing the dynamics of lobed radio sources are essential for
interpretation of the tens of millions of radio sources that will be observed by the Square …

Using a series of 3D relativistic hydrodynamical simulations of active galactic nuclei (AGN)
we investigate how AGN power, a clumpy interstellar medium (ISM) structure, and AGN jet …

Accreting supermassive black holes frequently power jets that interact with the interstellar
medium (ISM)/circumgalactic medium, regulating star formation in the galaxy. Highly …

We present the Cosmological Double Radio Active Galactic Nuclei (CosmoDRAGoN)
project: a large suite of simulated AGN jets in cosmological environments. These …

We present a method for applying spatially resolved adiabatic and radiative loss processes
to synthetic radio emission from hydrodynamic simulations of radio sources from active …

Abstract Using the Very Long Baseline Array, we observed the active galactic nucleus (AGN)
in NGC 3079 over a span of six months to test for variability in the two main parsec-scale …

Odd Radio Circles (ORCs) are a class of low surface brightness, circular objects
approximately one arcminute in diameter. ORCs were recently discovered in the Australian …

We present relativistic magnetohydrodynamic modelling of jets running into hydrostatic,
spherically symmetric cluster atmospheres. For the first time in a numerical simulation, we …

We study active galactic nucleus (AGN) feedback in nearby (z< 0.35) galaxy clusters from
the Planck Sunyaev–Zeldovich sample using Chandra observations. This nearly unbiased …