We present the PHANGS-MUSE survey, a programme that uses the MUSE integral field
spectrograph at the ESO VLT to map 19 massive (9.4< log (M⋆/M⊙)< 11.0) nearby (D≲ 20 …

We present a rich, multiwavelength, multiscale database built around the PHANGS–ALMA
CO (2− 1) survey and ancillary data. We use this database to present the distributions of …

We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct
morphological masks of sub-galactic environments based on Spitzer 3.6 μm images. At the …

Aims. The complexity of star formation at the physical scale of molecular clouds is not yet
fully understood. We investigate the mechanisms regulating the formation of stars in different …

We investigate the relationship between the star formation rate (SFR), stellar mass (M*), and
molecular gas mass () for local star-forming galaxies. We further investigate these …

Aims. We perform a homogeneous analysis of an unprecedented set of spatially resolved
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …

The feedback from young stars (ie pre-supernova) is thought to play a crucial role in
molecular cloud destruction. In this paper, we assess the feedback mechanisms acting …

We investigate the nature of the scaling relations between the surface density of star
formation rate (ΣSFR), stellar mass (Σ*), and molecular gas mass (), aiming at distinguishing …

Aims. We aim to constrain for the first time the mean mass and extent of the molecular gas of
a mass-complete sample of normal> 10 10 M⊙ star-forming galaxies at 0.4< z< 3.6 …

Feedback from an active galactic nucleus (AGN) is often implicated as a mechanism that
leads to the quenching of galactic star formation. However, AGN-driven quenching is …