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 …

In recent years, exciting developments have taken place in the identification of the role of
cosmic rays in star-forming environments. Observations from radio to infrared wavelengths …

We introduce a new model for the structure and evolution of the gas in galactic discs. In the
model the gas is in vertical pressure and energy balance. Star formation feedback injects …

We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct
morphological masks of sub-galactic environments based on Spitzer 3.6 μm images. At the …

Understanding the variability of galaxy star formation histories (SFHs) across a range of time-
scales provides insight into the underlying physical processes that regulate star formation …

The inner few hundred parsecs of the Milky Way harbours gas densities, pressures, velocity
dispersions, an interstellar radiation field and a cosmic ray ionization rate orders of …

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 …

Axion dark matter (DM) may efficiently convert to photons in the magnetospheres of neutron
stars (NSs), producing nearly monochromatic radio emission. This process is resonantly …

Evidence has mounted in recent decades that outflows of matter and energy from the central
few parsecs of our Galaxy have shaped the observed structure of the Milky Way on a variety …

ABSTRACT A key uncertainty in galaxy evolution is the physics regulating star formation,
ranging from small-scale processes related to the life-cycle of molecular clouds within …