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 …

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 …

The PHANGS collaboration has been building a reference data set for the multiscale,
multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With …

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 …

Massive, young stars are the main source of energy that maintains multiphase structure and
turbulence in the interstellar medium (ISM), and without this" feedback" the star formation …

Abstract PHANGS–JWST mid-infrared (MIR) imaging of nearby spiral galaxies has revealed
ubiquitous filaments of dust emission in intricate detail. We present a pilot study to …

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 …

Aims. In this Virgo Environment Traced in CO (VERTICO) science paper, we aim to study
how the star formation process depends on the galactic environment and gravitational …