Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

We present PHANGS–ALMA, the first survey to map CO J= 2→ 1 line emission at∼ 1''∼ 100
pc spatial resolution from a representative sample of 90 nearby (d≲ 20 Mpc) galaxies that lie …

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 present the characterization of the main properties of a sample of 98 AGN host galaxies,
both type-II and type-I, in comparison with those of≈ 2700 non-active galaxies observed by …

Star Formation Efficiency per Free-fall Time in nearby Galaxies - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …

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 …

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 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 …

Star formation is a multi-scale process that requires tracing cloud formation and stellar
feedback within the local (≲ kpc) and global galaxy environment. We present first results …