Polycyclic aromatic hydrocarbons (PAHs) play a critical role in the reprocessing of stellar
radiation and balancing the heating and cooling processes in the interstellar medium but …

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 …

In this work, we present a new catalogue of> 40 000 ionised nebulae distributed across the
19 galaxies observed by the PHANGS-MUSE survey. The nebulae have been classified …

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 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 …

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 …

Context. Stellar feedback in high-redshift galaxies plays an important, if not dominant, role in
the re-ionisation epoch of the Universe. Because of their extreme star formation (SF), the …

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 …

H ii region electron temperatures are a critical ingredient in metallicity determinations, and
recent observations have revealed systematic variations in the temperatures measured …

Results of a study of physical parameters of stellar population in star formation regions in
galaxies with signs of peculiarity NGC 3963 and NGC 7292 are presented. The study was …