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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 (2018)

First Author: Jackson J

Attributed to: Astrophysics Research at Liverpool John Moores University: Newly Appointed Academic Staff funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aae7c7

Publication URI: http://dx.doi.org/10.3847/1538-4357/aae7c7

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2