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 …

Non-thermal particles and high-energy radiation can play a role in the dynamical processes
in star-forming regions and provide an important piece of the multiwavelength observational …

It remains a major challenge to derive a theory of cloud-scale (pc) star formation and
feedback, describing how galaxies convert gas into stars as a function of the galactic …

Large-scale bars can fuel galaxy centers with molecular gas, often leading to the
development of dense ringlike structures where intense star formation occurs, forming a very …

The CO-to-H 2 conversion factor (α CO) is central to measuring the amount and properties of
molecular gas. It is known to vary with environmental conditions, and previous studies have …

Supernovae (SNe) dominate the energy and momentum budget of stellar feedback, but the
efficiency with which they couple to the interstellar medium (ISM) depends strongly on how …

We use hydrodynamical simulations to study the Milky Way's central molecular zone (CMZ).
The simulations include a non-equilibrium chemical network, the gas self-gravity, star …

A galaxy's morphology stems from the secular and environmental processes taking place
over the course of its evolutionary history. Thus, it has consistently served as an important …

ABSTRACT The Milky Way's Central Molecular Zone (CMZ) has emerged in recent years as
a unique laboratory for the study of star formation. Here we use the simulations presented in …

Context. The nuclear stellar disc (NSD) is, together with the nuclear star cluster (NSC) and
the central massive black hole, one of the main components in the central parts of our Milky …