162 citations · 1.1k across the 18 of their papers we have counts for
18 papers
The Three-mm Ultimate Mopra Milky Way Survey. III. Data Release 6, An Atlas of Physical Conditions, Global Mass Conversion Laws, and 3D Physical Architecture of the Molecular ISM in the Fourth Quadrant
Peter J. Barnes, Dylan G. H. Barnes, Audra K. Hernandez +2
We present Data Release 6 of ThrUMMS, consisting of complete data cubes and various moments of line emission (CO, CO, CO) from molecular clouds, across 60$^{\c…
A Search for 3-mm Molecular Absorption Line Transitions in the Magellanic Stream
Lucille Steffes, Daniel R. Rybarczyk, Snežana Stanimirović +14
The Magellanic Stream, a tidal tail of diffuse gas falling onto the Milky Way, formed by interactions between the Small and Large Magellanic Clouds, is primarily composed of neutra…
The SEDIGISM survey: first data release and overview of the Galactic structure
F. Schuller, J. S. Urquhart, T. Csengeri +57
The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium) survey used the APEX telescope to map 84 deg^2 of the Galactic plane between l = -60 deg…
The integrated properties of the molecular clouds from the JCMT CO(3-2) High Resolution Survey
Dario Colombo, Erik Rosolowsky, Ana Duarte-Cabral +6
We define the molecular cloud properties of the Milky Way first quadrant using data from the JCMT CO(3-2) High Resolution Survey. We apply the Spectral Clustering for Interstellar…
The Galactic Census of High- and Medium-mass Protostars. IV. Molecular Clump Radiative Transfer, Mass Distributions, Kinematics, and Dynamical Evolution
Peter J. Barnes, Audra K. Hernandez, Erik Muller +1
We present CO, CO, and CO data as the next major release for the CHaMP project, an unbiased sample of Galactic molecular clouds in = 280-300$^{\c…
SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium
F. Schuller, T. Csengeri, J. S. Urquhart +41
The origin and life-cycle of molecular clouds are still poorly constrained, despite their importance for understanding the evolution of the interstellar medium. We have carried out…