Galaxy-scale outflows of gas, or galactic winds (GWs), driven by energy from star formation
are a pivotal mechanism for regulation of star formation in the current model of galaxy …

We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …

There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …

We study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158
μm emission in a large sample of normal star-forming galaxies at 4< z< 6 from the ALMA …

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 …

We examine the connection between the properties of the circumgalactic medium (CGM)
and the quenching and morphological evolution of central galaxies in the EAGLE and …

We present results from our on-going MusE GAs FLOw and Wind (MEGAFLOW) survey,
which consists of 22 quasar lines of sight, each observed with the integral field unit MUSE …

By using a set of different star formation rate (SFR) indicators, including Wide-field Infrared
Survey Explorer (WISE) mid-infrared and H α emission, we study the slope of the main …

Feedback by Massive Black Holes in Gas-rich Dwarf Galaxies - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …

The global influence of AGN-driven outflows remains uncertain, due to a lack of large
samples with accurately determined outflow properties. In the second paper of this series …