Outflows from active galactic nuclei (AGNs) are one of the fundamental mechanisms by
which the central supermassive black hole interacts with its host galaxy. Detected in≥ 50 …

Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …

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

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 …

Insights from JWST observations suggest that active galactic nuclei feedback evolved from a
short-lived, high-redshift phase in which radiatively cooled turbulence and/or momentum …

Supermassive black holes are found at the centres of massive galaxies. During the growth of
these black holes they light up to become visible as active galactic nuclei (AGNs) and …

We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6< z< 2.7,
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …

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 …

Mrk 231 is a nearby ultra-luminous IR galaxy exhibiting a kpc-scale, multi-phase AGN-driven
outflow. This galaxy represents the best target to investigate in detail the morphology and …

Aims. Outflows driven by active galactic nuclei (AGN) are invoked by galaxy evolutionary
models to quench star formation and to explain the origin of the relations observed locally …