There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …

We use integral field spectroscopy from the PHANGS–MUSE survey, which resolves the
ionised interstellar medium structure at∼ 50 pc resolution in 19 nearby spiral galaxies, to …

The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with
KMOS3D - IOPscience This site uses cookies. By continuing to use this site you agree to our …

We present kinematic orientations and high-resolution (150 pc) rotation curves for 67 main-
sequence star-forming galaxies surveyed in CO (2–1) emission by PHANGS–ALMA. Our …

We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of 86
nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses …

We compare the molecular and ionized gas velocity dispersions of nine nearby turbulent
disks, analogs to high-redshift galaxies, from the DYNAMO sample using new 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 …

We measure the molecular-to-atomic gas ratio, R mol, and the star formation rate (SFR) per
unit molecular gas mass, SFE mol, in 38 nearby galaxies selected from the Virgo …

Context. Spatially resolved studies of the kinematics of galaxies provide crucial insights into
their assembly and evolution, enabling one to infer the properties of the dark matter halos …

Context. Theoretical models struggle to reproduce dynamically cold disks with significant
rotation-to-dispersion support (V rot/σ) observed in star-forming galaxies in the early …