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 driven by jets from active galactic nuclei is believed to be responsible for reducing
cooling flows in cool-core galaxy clusters. We use simulations to model feedback from …

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 …

Radio galaxies in clusters of galaxies are a prominent reservoir of magnetic fields and of
non-thermal particles, which become mixed with the intracluster medium. We review the …

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 …

Active galactic nuclei (AGNs) play an integral role in galaxy formation and evolution by
influencing galaxies and their environments through radio jet feedback. Historically …

We investigate the evolution of active galactic nucleus jets on kiloparsec-scales due to their
interaction with the clumpy interstellar medium (ISM) of the host galaxy and, subsequently …

The study of radio galaxies (RGs) offers valuable insights into the complex dynamics
between active galactic nuclei (AGN), host galaxies, and the surrounding medium. Among …