The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …

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 …

Using a sample of∼ 15 000 kpc-scale star-forming spaxels in 28 galaxies drawn from the
ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we investigate the …

We study the global star formation rate (SFR) versus stellar mass (M*) correlation, and the
spatially resolved SFR surface density (ΣSFR) versus stellar mass surface density (Σ*) …

Using a sample of 11 478 spaxels in 34 galaxies with molecular gas, star formation, and
stellar maps taken from the ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) …

Abstract The ALMaQUEST (ALMA-MaNGA QUEnching and STar formation) survey is a
program with spatially resolved 12 CO (1− 0) measurements obtained with the Atacama …

We present a new characterization of the relations between star-formation rate, stellar mass,
and molecular gas mass surface densities at different spatial scales across galaxies (from …

Aims. There exists some consensus that the stellar mass surface density (Σ⋆) and molecular
gas mass surface density (Σ mol) are the main quantities responsible for locally setting the …

The origin of the star-forming main sequence (SFMS; ie, the relation between star formation
rate and stellar mass, globally or on kpc scales) remains a hotly debated topic in galaxy …