Suzanne Madden
0000-0003-3229-2899
11 papers found
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The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral Atomic Carbon [C i]
An ALMA View of Molecular Filaments in the Large Magellanic Cloud. I. The Formation of High-mass Stars and Pillars in the N159E-Papillon Nebula Triggered by a Cloud–Cloud Collision
An ALMA View of Molecular Filaments in the Large Magellanic Cloud. II. An Early Stage of High-mass Star Formation Embedded at Colliding Clouds in N159W-South
A Survey of Atomic Carbon [C i] in High-redshift Main-sequence Galaxies
ALMA Reveals Molecular Cloud N55 in the Large Magellanic Cloud as a Site of Massive Star Formation
Dust Emission at 8 and 24μm as Diagnostics of H ii Region Radiative Transfer
Erratum: “Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission” (2014, ApJ, 797, 85)
Kinematic Structure of Molecular Gas Around High-Mass Yso, Papillon Nebula, in N159 East in the Large Magellanic Cloud: A New Perspective With Alma
The RELATIONSHIP BETWEEN MOLECULAR GAS, H I, AND STAR FORMATION IN THE LOW-MASS, LOW-METALLICITY MAGELLANIC CLOUDS
The Dense Gas in the Largest Molecular Complexes of the Antennae: Hcn and Hco+observations of Ngc 4038/39 Using Alma
High-Mass Star Formation Triggered by Collision Between Co Filaments in N159 West in the Large Magellanic Cloud
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