The universe's biggest galaxies have both vast atmospheres and supermassive central
black holes. This article reviews how those two components of a large galaxy couple and …

Formation of galaxy clusters corresponds to the collapse of the largest gravitationally bound
overdensities in the initial density field and is accompanied by the most energetic …

Cosmological simulations are an important theoretical pillar for understanding non-linear
structure formation in our Universe and for relating it to observations on large scales. In …

Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as
the main mechanism responsible for regulating star formation in active galactic nucleus …

The radiative cooling timescales at the centers of hot atmospheres surrounding elliptical
galaxies, groups and clusters are much shorter than their ages. Therefore, hot atmospheres …

The co-evolution between supermassive black holes and their environment is most directly
traced by the hot atmospheres of dark matter halos. The cooling of the hot atmosphere …

We introduce the Cluster-EAGLE (c-eagle) simulation project, a set of cosmological
hydrodynamical zoom simulations of the formation of 30 galaxy clusters in the mass range of …

We present a new suite of large-volume cosmological hydrodynamical simulations called
cosmo-OWLS. They form an extension to the OverWhelmingly Large Simulations (OWLS) …

Using Chandra X-ray and Very Large Array radio data, we investigate the scaling
relationship between jet power, P jet, and synchrotron luminosity, P radio. We expand the …

Galactic outflows are ubiquitous in galaxies containing active star formation or supermassive
black hole activity. The presence of a large-scale outflow from the center of our own Galaxy …