CO line emission represents the most accessible and widely used tracer of the molecular
ISM. This renders the translation of observed CO intensity into total H2 gas mass critical to …

Measurements of H α, HI, and CO distributions in 61 normal spiral galaxies are combined
with published far-infrared and CO observations of 36 infrared-selected starburst galaxies, in …

We present models of photometric evolution of galaxies in which the effects of a dusty
interstellar medium have been included with particular care. A chemical evolution code …

We present models for the evolution of the elemental abundances in the gas and dust
phases of the interstellar medium (ISM) of our Galaxy by generalizing standard models for its …

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 …

Photodissociation region (PDR) models are computed over a wide range of physical
conditions, from those appropriate to giant molecular clouds illuminated by the interstellar …

We report the results of a pilot study with the Expanded Very Large Array (EVLA) of 12CO J=
1–0 emission from four submillimetre-selected galaxies at z= 2.2–2.5, each with an existing …

We use the first systematic samples of CO millimeter emission in z⩾ 1''main-sequence''star-
forming galaxies to study the metallicity dependence of the conversion factor α CO, from CO …

We present a wide area (≈ 8× 8 kpc), sensitive map of CO (2–1) emission around the
nearby starburst galaxy M82. Molecular gas extends far beyond the stellar disk, including …

We study the properties of the cold gas component of the interstellar medium of the Herschel
Reference Survey, a complete volume-limited (15≲ D≲ 25 Mpc), K-band-selected sample of …