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ALMA-IMF II -- investigating the origin of stellar masses: Continuum Images and Data Processing
A. Ginsburg, T. Csengeri, R. Galván-Madrid +49
We present the first data release of the ALMA-IMF Large Program, which covers the 12m-array continuum calibration and imaging. The ALMA-IMF Large Program is a survey of fifteen den…
Structure of the Source I disk in Orion-KL
Melvyn Wright, John Baly, Tomoya Hirota +6
This paper analyses images from 43 to 340 GHz to trace the structure of the Source I disk in Orion-KL with 12 AU resolution. The data reveal an almost edge-on disk with an ou…
The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way
D. Colombo, A. Duarte-Cabral, A. R. Pettitt +23
The morphology of the Milky Way is still a matter of debate. In order to shed light on uncertainties surrounding the structure of the Galaxy, in this paper, we study the imprint of…
Small Protoplanetary Disks in the Orion Nebula Cluster and OMC1 with ALMA
Justin Otter, Adam Ginsburg, Nicholas P. Ballering +5
The Orion Nebula Cluster (ONC) is the nearest dense star-forming region at 400 pc away, making it an ideal target to study the impact of high stellar density and proximity to…
Are massive dense clumps truly sub-virial? A new analysis using Gould Belt ammonia data
Ayushi Singh, Christopher D. Matzner, Rachel K. Friesen +21
Dynamical studies of dense structures within molecular clouds often conclude that the most massive clumps contain too little kinetic energy for virial equilibrium, unless they are…
A Core Mass Function Indistinguishable from the Salpeter Stellar Initial Mass Function Using 1000 au Resolution ALMA Observations
Genaro Suárez, Roberto Galván-Madrid, Luis Aguilar +4
We present the core mass function (CMF) of the massive star-forming clump G33.92+0.11 using 1.3 mm observations obtained with the Atacama Large Millimeter/submillimeter Array (ALMA…