Group Publications For Download
Highlights
Mills et al. 2018a: The dense gas fraction is measured to increase with proximity to the Galactic center. Clouds in the inner 100 pc are characterized by at least two excitation components: the bulk of the gas has densities of ~10^3 per cm^3 with only ~15% of the gas at densities higher than 10^5 per cm^3.
Galactic center
CMZoom. IV. Incipient High-mass Star Formation throughout the Central Molecular Zone
JWST Reveals Widespread CO Ice and Gas Absorption in the Galactic Center Cloud G0.253+0.016
CMZoom III: Spectral line data release
ALMA Uncovers Highly Filamentary Structure toward the Sgr E Region
The initial conditions for young massive cluster formation in the Galactic Centre: convergence of large-scale gas flows
A wind-blown bubble in the Central Molecular Zone cloud G0.253+0.016
Star formation in 'the Brick': ALMA reveals an active protocluster in the Galactic centre cloud G0.253+0.016
ALMA Observations of Massive Clouds in the Central Molecular Zone: Ubiquitous Protostellar Outflows
CMZoom. II. Catalog of Compact Submillimeter Dust Continuum Sources in the Milky Way's Central Molecular Zone
CMZoom: Survey Overview and First Data Release
The Turbulent Gas Structure in the Centers of NGC 253 and the Milky Way
SOFIA/FORCAST Galactic Center Legacy Survey: Overview
A Census of Early-phase High-mass Star Formation in the Central Molecular Zone
Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds
`The Brick' is not a brick: a comprehensive study of the structure and dynamics of the central molecular zone cloud G0.253+0.016
SOFIA/FORCAST Observations of the Sgr A-H H II Regions: Using Dust Emission to Elucidate the Heating Sources
The dynamical evolution of molecular clouds near the Galactic Centre - II. Spatial structure and kinematics of simulated clouds
Star Formation Rates of Massive Molecular Clouds in the Central Molecular Zone
Discovery of 14NH3 (2,2) Maser Emission in Sgr B2 Main
A Centimeter-wave Study of Methanol and Ammonia Isotopologues in Sgr B2(N): Physical and Chemical Differentiation between Two Hot Cores
The Dense Gas Fraction in Galactic Center Clouds
Star formation in a high-pressure environment: an SMA view of the Galactic Centre dust ridge
Distributed Star Formation throughout the Galactic Center Cloud Sgr B2
M0.20-0.033: An Expanding Molecular Shell in the Galactic Center Radio Arc
Hot Molecular Gas in the Circumnuclear Disk
Nearby Galaxies
[C II] Spectral Mapping of the Galactic Wind and Starbursting Disk of M82 with SOFIA
The Morpho-kinematic Architecture of Super Star Clusters in the Center of NGC 253
ALMA Imaging of a Galactic Molecular Outflow in NGC 4945
Clustered Star Formation in the Center of NGC 253 Contributes to Driving the Ionized Nuclear Wind
Outflows from Super Star Clusters in the Central Starburst of NGC 253
The Turbulent Gas Structure in the Centers of NGC 253 and the Milky Way
The Molecular Interstellar Medium in the Super Star Clusters of the Starburst NGC 253
The Molecular Outflow in NGC 253 at a Resolution of Two Parsecs
Forming Super Star Clusters in the Central Starburst of NGC 253
Spatially Resolved 12CO(2-1)/12CO(1-0) in the Starburst Galaxy NGC 253: Assessing Optical Depth to Constrain the Molecular Mass Outflow Rate
Molecular gas in the northern nucleus of Mrk 273: Physical and chemical properties of the disc and its outflow
Star Formation
Stellar Properties
Unusual Isotopic Abundances in a Fully Convective Stellar Binary
Far-Infrared Facilities and Technology Development
Review: far-infrared instrumentation and technological development for the next decade