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 …

Core-collapse supernovae are explosions of massive stars at the end of their evolution.
They are responsible for metal production and for halting star formation, having a significant …

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 …

We present a chemical analysis of selected H II regions from the PHANGS-MUSE nebular
catalogue. Our intent is to empirically re-calibrate strong-line diagnostics of gas-phase …

The evolution of giant molecular clouds (GMCs), the main sites of high-mass star formation,
is an essential process to unravel the galaxy evolution. Using a GMC catalogue of M 33 from …

We present the Physics at High Angular resolution in Nearby GalaxieS (PHANGS)-AstroSat
atlas, which contains UV imaging of 31 nearby star-forming galaxies captured by the …

Aims. We analyse synthetic emission maps of the [CII] 158 µm line and far-infrared (FIR)
continuum of simulated molecular clouds (MCs) within the SILCC-Zoom project to study the …

The ionizing radiation of young and massive stars is a crucial form of stellar feedback. Most
ionizing (Lyman-continuum; LyC, λ< 912Å) photons are absorbed close to the stars that …

The variations of oxygen abundance and ionization parameter in H ii regions are usually
thought to be the dominant factors that produced variations seen in observed emission-line …

We present the results of a study of young unresolved stellar groupings (clusters, OB
associations, and their complexes) associated with H ii regions, based on the coupling of …