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Star-Forming Filaments and Cores in Molecular Clouds

Published onMay 31, 2019
Star-Forming Filaments and Cores in Molecular Clouds
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Abstract

Dense, star-forming gas in molecular clouds is dominated by filamentary structures. We describe the best probes of the dynamics of filaments and cores in nearby star-forming molecular clouds, and our recommendations for furthering our understanding of star formation physics through observations over the next decade.

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