Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …

ABSTRACT NGC 1266 is a nearby lenticular galaxy that harbors a massive outflow of
molecular gas powered by the mechanical energy of an active galactic nucleus (AGN). It has …

We present results from the James Webb Space Telescope Director's Discretionary Time
Early Release Science program 1328 targeting the nearby, luminous infrared galaxy, VV …

For the first time, we reveal large amounts of cold molecular gas in a ram-pressure-stripped
tail, out to a large" intracluster" distance from the galaxy. With the Actama Pathfinder …

Abstract We combine James Webb Space Telescope (JWST) and Hubble Space Telescope
imaging with Atacama Large Millimeter Array CO (2–1) spectroscopy to study the highly …

Starburst galaxies at the peak of cosmic star formation are among the most extreme star-
forming engines in the Universe, producing stars over about 100 million years (ref.). The star …

Context. Large-scale motions in galaxies (supernovae explosions, galaxy collisions, galactic
shear etc.) generate turbulence, which allows a fraction of the available kinetic energy to …

We present the first Herschel spectroscopic detections of the [O i] 63 μm and [C ii] 158 μm
fine-structure transitions, and a single para-H 2 O line from the 35× 15 kpc 2 shocked …

Line ratio diagnostics provide valuable clues as to the source of ionizing radiation in
galaxies with intense black hole accretion and starbursting events, such as local Seyfert …

We have recently detected the [C ii] 157.7 μm line in eight star-forming galaxies at redshifts 1
to 2 using the redshift (z) Early Universe Spectrometer (ZEUS). Our sample targets star …