We review progress over the past decade in observations of large-scale star formation, with
a focus on the interface between extragalactic and Galactic studies. Methods of measuring …

Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved
studies of the interstellar medium, star formation and nuclear activity across a broad range of …

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 …

Mergers of galaxies are thought to cause significant gas inflows to the inner parsecs, which
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …

We report subarcsecond resolution IRAM PdBI millimeter CO interferometry of four z\sim 2
submillimeter galaxies (SMGs), and sensitive CO (3-2) flux limits toward three z\sim 2 …

Measurements of interstellar Na I λλ5890, 5896 absorption lines in 18 ultraluminous infrared
galaxies (ULIGs) have been combined with published Na I data, to reassess the …

Massive, galaxy-scale outflows are known to be ubiquitous in major mergers of disk galaxies
in the local universe. In this paper, we explore the multiphase structure and power sources …

We report the results from a comprehensive study of 74 ultraluminous infrared galaxies
(ULIRGs) and 34 Palomar-Green (PG) quasars within z∼ 0.3 observed with the Spitzer …

Enhanced Subkiloparsec-scale Star Formation: Results from a JWST Size Analysis of 341
Galaxies at 5 < z < 14 - IOPscience This site uses cookies. By continuing to use this site you …

Luminous infrared starbursts in the early Universe are thought to be the progenitors of
massive quiescent galaxies identified at redshifts 2–4. Using the Mid-IRfrared Instrument …