The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …

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 …

Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …

Context. Molecular gas is a necessary fuel for star formation. The CO (1− 0) transition is
often used to deduce the total molecular hydrogen but is challenging to detect in low …

Most of the celestial γ rays detected by the Large Area Telescope (LAT) on board the Fermi
Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic …

The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …

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 explore the kinematics of 27 z≳ 6 quasar host galaxies observed in [C ii] 158 μm ([C ii])
emission with the Atacama Large Millimeter/submillimeter Array at a resolution of≈ 025. We …

We present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …

We present the ancillary data and basic physical measurements for the galaxies in the
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …