Jill Rathborne
0000-0002-3427-9092
11 papers found
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Asymmetric Line Profiles in Dense Molecular Clumps Observed in MALT90: Evidence for Global Collapse
G337.342–0.119 (The “Pebble”): A Cold, Dense, High-mass Molecular Cloud with Unusually Large Line Widths and a Candidate High-mass Star Cluster Progenitor
The Radio Ammonia Mid-plane Survey (RAMPS) Pilot Survey
MALT90 Kinematic Distances to Dense Molecular Clumps
The Link Between Turbulence, Magnetic Fields, Filaments, and Star Formation in the Central Molecular Zone Cloud G0.253+0.016
Linking Dense Gas From the Milky Way to External Galaxies
Far-Infrared Dust Temperatures and Column Densities of the Malt90 Molecular Clump Sample
A Cluster in the Making: Alma Reveals the Initial Conditions for High-Mass Cluster Formation
Turbulence Sets the Initial Conditions for Star Formation in High-Pressure Environments
Absorption Filaments Toward the Massive Clump G0.253+0.016
Distributed Low-Mass Star Formation in the Irdc G34.43+00.24
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