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(s):: 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.

Published: 2018
Publication type: Article / Letter to editor

Date issued: 2018
Language: English
Is part of: Astrophysical Journal (2018), Vol. 869, no. 2, p. 102
hdl: 1887/69537
doi: 10.3847/1538-4357/aae7c7
URL: https://ui.adsabs.harvard.edu/#abs/2018ApJ...869..102J