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 …

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 introduce a new suite of simulations,'The Cloud Factory', which self-consistently forms
molecular cloud complexes at high enough resolution to resolve internal substructure (up to …

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 …

Abstract The Galactic Centre contains a supermassive black hole with a mass of four million
Suns within an environment that differs markedly from that of the Galactic disk. Although the …

Within the central few hundred parsecs of the Milky Way, extending from longitude l=− 1° to
1.5°, lies the Central Molecular Zone of the Galactic Centre. This extraordinary region is …

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 present here the first of a series of papers aimed at better understanding the evolution
and properties of giant molecular clouds (GMCs) in a galactic context. We perform high …

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 …