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

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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

Type: Article / Letter to editor
Title: 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
Author: Jackson, J.M.Contreras, Morales Y.Rathborne, J.M.Whitaker.J.S.Guzmán, A.Stephens, I.W.Sanhueza, P.Longmore, S.Zhang, Q.Allingham, D.
Journal Title: Astrophysical Journal
Issue: 2
Volume: 869
Start Page: 102
Issue Date: 2018
Uri: https://ui.adsabs.harvard.edu/#abs/2018ApJ...869..102J
Handle: http://hdl.handle.net/1887/69537
 

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