Observations that resolve nearby galaxies into individual regions across multiple phases of
the gas–star formation feedback “matter cycle” have provided a sharp new view of molecular …

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 …

Large-scale outflows in star-forming galaxies are observed to be ubiquitous and are a key
aspect of theoretical modeling of galactic evolution, the focus of the Simulating Multiscale …

Abstract Using the PHANGS–ALMA CO (2–1) survey, we characterize molecular gas
properties on∼ 100 pc scales across 102,778 independent sightlines in 70 nearby galaxies …

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 …

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 …

We determine radial velocities and mass flow rates in a sample of 54 local spiral galaxies by
modeling high-resolution and high-sensitivity data of the atomic hydrogen emission line. We …

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 …

It is widely known that the gas in galaxy discs is highly turbulent, but there is much debate on
which mechanism can energetically maintain this turbulence. Among the possible …

Galactic bars can drive cold gas inflows towards the centres of galaxies. The gas transport
happens primarily through the so-called bar dust lanes, which connect the galactic disc at …