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 …

It is a major open question which physical processes stop gas accretion on to giant
molecular clouds (GMCs) and limit the efficiency at which gas is converted into stars. While …

The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic
disks, but the detailed gas phase metallicity distribution remains poorly sampled. We have …

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 …

Abstract The Sloan Digital Sky Survey IV Mapping Nearby Galaxies at APO (MaNGA)
program has been operating from 2014 to 2020, and has now observed a sample of 9269 …

The nebular recombination line H α is widely used as a star formation rate (SFR) indicator in
the local and high-redshift Universe. We present a detailed H α radiative transfer study of …

We present an analysis of the diffuse ionized gas (DIG) in a high-resolution simulation of an
isolated Milky Way-like galaxy, incorporating on-the-fly radiative transfer and non …

Context. Stellar feedback is a key contributor to the morphology and dynamics of the
interstellar medium in star-forming galaxies. In particular, energy and momentum input from …

We use the statistical power of the MaNGA integral-field spectroscopic galaxy survey to
improve the definition of strong line diagnostic boundaries used to classify gas ionization …

We present morphological classifications of∼ 27 million galaxies from the Dark Energy
Survey (DES) Data Release 1 (DR1) using a supervised deep learning algorithm. The …