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 …

Context. Stellar feedback is a key contributor to the morphology and dynamics of the
interstellar medium in star-forming galaxies. In particular, energy and momentum input from …

We present a high-resolution view of bubbles within the Phantom Galaxy (NGC 628), a
nearby (∼ 10 Mpc), star-forming (∼ 2 M⊙ yr− 1), face-on (i∼ 9) grand-design spiral galaxy …

Context. Energy and momentum injected by young, massive stars into the surrounding gas
play an important role in regulating further star formation and in determining the galaxy's …

Polycyclic aromatic hydrocarbons (PAHs) are a ubiquitous component of the interstellar
medium (ISM) in z∼ 0 massive, star-forming galaxies and play key roles in ISM energy …

The molecular-to-atomic gas ratio is crucial to our understanding of the evolution of the
interstellar medium (ISM) in galaxies. We investigated the balance between the atomic (Σ HI) …

We present the largest catalog to date of star clusters and compact associations in nearby
galaxies. We have performed a V-band-selected census of clusters across the 38 spiral …

Abstract We employ the Feedback In Realistic Environments (FIRE-2) physics model to
study how the properties of giant molecular clouds (GMCs) evolve during galaxy mergers …

We compare mid-infrared (mid-IR), extinction-corrected Hα, and CO (2–1) emission at 70–
160 pc resolution in the first four PHANGS–JWST targets. We report correlation strengths …

Connecting the gas in H ii regions to the underlying source of the ionizing radiation can help
us constrain the physical processes of stellar feedback and how H ii regions evolve over …