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)
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