Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …

The energy released by Active Galactic Nuclei (AGN) in the form of radiation, winds, or radio
plasma jets, is known to impact on the surrounding interstellar medium. The result of these …

The inefficiency of star formation in massive elliptical galaxies is widely believed to be
caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas …

Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …

Hydrodynamical cosmological simulations are increasing their level of realism by
considering more physical processes and having greater resolution or larger statistics …

We study molecular outflows in a sample of 45 local galaxies, both star forming and active
galactic nucleus (AGN), primarily by using CO data from the Atacama Large Millimeter …

Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the
quenching of massive galaxies in the vast majority of modern galaxy evolution models …

We study the interactions of a relativistic jet with a dense turbulent gaseous disc of radius∼
2 kpc. We have performed a suite of simulations with different mean density, jet power, and …

Reionization in the early Universe is likely driven by dwarf galaxies. Using cosmological
radiation-hydrodynamic simulations, we study star formation and the escape of Lyman …

The discovery of quasars a few hundred megayears after the Big Bang represents a major
challenge to our understanding of black holes as well as galaxy formation and evolution …