activity
20022013
most citedThe Herschel view of massive star formation in G035.39--00.33: Dense and cold filament of W48 undergoing a mini-starburst

115 citations · 458 across the 10 of their papers we have counts for

collaborators
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6 papers · 1 filter

astro-ph2007★ 13 cited

Deconstructing the High-Mass Star-Forming Region IRAS 23033+5951

Michael A. Reid, Brenda C. Matthews

We report interferometric observations of the high-mass star-forming object IRAS 23033+5951. Our observations reveal two massive molecular cloud cores, designated IRAS 23033+5951-M…

astro-ph2006★ 54 cited

High Mass Star Formation. III. The Functional Form of the Submillimeter Clump Mass Function

Michael A. Reid, Christine D. Wilson

We investigate the mass function of cold, dusty clumps in 11 low- and high-mass star-forming regions. Using a homogeneous fitting technique, we analyze the shape of each region's c…

astro-ph2006★ 58 cited

High Mass Star Formation. II. The Mass Function of Submillimeter Clumps in M17

M. A. Reid, C. D. Wilson

We have mapped an approximately 5.5 by 5.5 pc portion of the M17 massive star-forming region in both 850 and 450 micron dust continuum emission using the Submillimeter Common-User…

astro-ph2005★ 93 cited

High Mass Star Formation I: The Mass Distribution of Submillimeter Clumps in NGC 7538

M. A. Reid, C. D. Wilson

We present submillimeter continuum maps at 450 and 850 microns of a 12 x 8 arcminute region of the NGC 7538 high-mass star-forming region, made using the Submillimeter Common-User…

astro-ph2002

Star Formation: 3D Collapse of Turbulent Cloud Cores

M. A. Reid, R. E. Pudritz, J. Wadsley

We have performed fully 3D simulations of the collapse of molecular cloud cores which obey the logatropic equation of state. By following the collapse of these cores from states of…

astro-ph2002★ 7 cited

3-D Simulations of the Gravitational Collapse of Logatropic Molecular Cloud Cores

M. A. Reid, R. E. Pudritz, J. Wadsley

We present the results of fully 3-D hydrodynamic simulations of the gravitational collapse of isolated, turbulent molecular cloud cores. Starting from initial states of hydrostatic…