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American Astronomical Society, Astrophysical Journal, 2(869), p. 102, 2018

DOI: 10.3847/1538-4357/aae7c7

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G337.342–0.119 (The “Pebble”): A Cold, Dense, High-mass Molecular Cloud with Unusually Large Line Widths and a Candidate High-mass Star Cluster Progenitor

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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