We present a spatially resolved study of the kinematical properties of known supernova
remnants (SNRs) in the nearest galaxies of the SIGNALS survey, namely NGC 6822 (one …

We present the Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS)
project, designed for the spatial and spectral study of the diffuse ionised gas (DIG) in a …

Context. A reliable molecular clump detection algorithm is essential for studying these
clumps. Existing detection algorithms for molecular clumps still require that detected …

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 …

Supernova feedback injects energy and turbulence into the interstellar medium (ISM) in
galaxies, influences the process of star formation, and is essential to understanding the …

In this study, we use MUSE Integral Field Spectroscopy (IFS), along with multiline
diagnostics, for the optical identification of supernova remnants (SNRs) in the galaxy NGC …

We examine the connection between diffuse ionized gas (DIG), H ii regions, and field O and
B stars in the nearby spiral M101 and its dwarf companion NGC 5474 using ultra-deep H α …

The nearby irregular galaxy NGC 4449 has a star formation rate of∼ 0.4M☉ yr− 1 and
should host of order 70 supernova remnants (SNRs) younger than 20,000 yr, a typical age …

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

Classifying ionised nebulae in nearby galaxies is crucial to studying stellar feedback
mechanisms and understanding the physical conditions of the interstellar medium. This …