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Using Molecular Gas Observations to Guide Initial Conditions for Star Cluster Simulations
Alison Sills, Steven Rieder, Anne S. M. Buckner +3
The earliest evolution of star clusters involves a phase of co-existence of both newly-formed stars, and the gas from which they are forming. Observations of the gas in such region…
The 30 Doradus Molecular Cloud at 0.4 pc Resolution with the Atacama Large Millimeter/submillimeter Array: Physical Properties and the Boundedness of CO-emitting Structures
Tony Wong, Luuk Oudshoorn, Eliyahu Sofovich +21
We present results of a wide-field (approximately 60 x 90 pc) ALMA mosaic of CO(2-1) and CO(2-1) emission from the molecular cloud associated with the 30 Doradus star-formin…
Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
A. Hacar, S Clark, F. Heitsch +4
The interstellar medium contains filamentary structure over a wide range of scales. Understanding the role of this structure, both as a conduit of gas across the scales and a diagn…
Survey of Orion Disks with ALMA (SODA) I: Cloud-level demographics of 873 protoplanetary disks
S. E. van Terwisga, A. Hacar, E. F. van Dishoeck +2
(Abridged) Surveys of protoplanetary disks in nearby star-forming regions (SFRs) have provided important information on their demographics, but due to their sample sizes, they cann…