Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …

Observations that resolve nearby galaxies into individual regions across multiple phases of
the gas–star formation feedback “matter cycle” have provided a sharp new view of molecular …

We use deep JWST/NIRSpec R∼ 1000 slit spectra of 113 galaxies at, selected from the
mass-complete Blue Jay survey, to investigate the prevalence and typical properties of …

Feedback to the interstellar medium from ionizing radiation, stellar winds and supernovae is
central to regulating star formation in galaxies. Owing to their low mass (< 109 solar …

Massive galaxy-scale outflows of gas are one of the most commonly invoked mechanisms to
regulate the growth and evolution of galaxies throughout the universe. While the gas in …

We study star formation-driven outflows in az∼ 0.02 starbursting disc galaxy, IRAS08339+
6517, using spatially resolved measurements from the Keck Cosmic Web Imager (KCWI) …

Context. The interstellar medium is the locus of physical processes affecting the evolution of
galaxies which drive or are the result of star formation activity, supermassive black hole …

We analyze image and spectral data from≈ 365 ks of observations from the Chandra X-ray
Observatory of the nearby, edge-on starburst galaxy NGC 253 to constrain properties of the …

The center of the nearby galaxy NGC 253 hosts a population of more than a dozen super
star clusters (SSCs) that are still in the process of forming. The majority of the star formation …

Context. Observations of chemical species can provide insights into the physical conditions
of the emitting gas however it is important to understand how their abundances and …