Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

▪ Abstract Galactic winds are the primary mechanism by which energy and metals are
recycled in galaxies and are deposited into the intergalactic medium. New observations are …

We study molecular outflows in a sample of 45 local galaxies, both star forming and active
galactic nucleus (AGN), primarily by using CO data from the Atacama Large Millimeter …

We use the first systematic data sets of CO molecular line emission in z∼ 1–3 normal star-
forming galaxies (SFGs) for a comparison of the dependence of galaxy-averaged star …

We present the deepest 100 to 500 μm far-infrared observations obtained with the Herschel
Space Observatory as part of the GOODS-Herschel key program, and examine the infrared …

We report the results from a systematic search for molecular (OH 119 μm) outflows with
Herschel/PACS in a sample of 43 nearby (z< 0.3) galaxy mergers, mostly ultraluminous …

HCN luminosity is a tracer of dense molecular gas, n (H 2)≳ 3× 10 4 cm-3, associated with
star-forming giant molecular cloud (GMC) cores. We present the results and analysis of our …

We use spectra from the ALFALFA, GASS and COLD GASS surveys to quantify variations in
the mean atomic and molecular gas mass fractions throughout the SFR–M* plane and along …

Collisions and interactions between gas-rich galaxies are thought to be pivotal stages in
their formation and evolution, causing the rapid production of new stars, and possibly …

The role of galaxy mergers in fuelling active galactic nuclei (AGNs) is still debated, owing
partly to selection effects inherent to studies of the merger/AGN connection. In particular …