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Physical Conditions and Kinematics of the Filamentary Structure in Orion Molecular Cloud 1

14 May 2020, 16:00 UTC
Physical Conditions and Kinematics of the Filamentary Structure in Orion Molecular Cloud 1
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Yu-Hsuan Teng and Naomi Hirano 2020 ApJ 893 63
Observations of the Orion Molecular Cloud 1 with the Submillimeter Array and the Submillimeter Telescope reveal multiple filaments of dense gas with typical width of 0.02–0.03 pc collapsing toward the Orion Nebula Cluster.

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