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 …

We present a rich, multiwavelength, multiscale database built around the PHANGS–ALMA
CO (2− 1) survey and ancillary data. We use this database to present the distributions of …

The processes of star formation and feedback, regulating the cycle of matter between gas
and stars on the scales of giant molecular clouds (GMCs;∼ 100 pc), play a major role in …

We measure empirical relationships between the local star formation rate (SFR) and
properties of the star-forming molecular gas on 1.5 kpc scales across 80 nearby galaxies …

We present maps tracing the fraction of dust in the form of polycyclic aromatic hydrocarbons
(PAHs) in IC 5332, NGC 628, NGC 1365, and NGC 7496 from JWST/MIRI observations. We …

We present the CO isotopologue Line Atlas within the Whirpool galaxy Survey (CLAWS),
which is based on an IRAM 30 m large programme that provides a benchmark study of …

Ratios of polycyclic aromatic hydrocarbon (PAH) vibrational bands are a promising tool for
measuring the properties of the PAH population and their effect on star formation. The …

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 …

JWST observations of polycyclic aromatic hydrocarbon (PAH) emission provide some of the
deepest and highest resolution views of the cold interstellar medium (ISM) in nearby …

We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of 86
nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses …