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-Reference-Cited by-同舟云学术

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

Published:2018-12-14 Issue:2 Volume:869 Page:102
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Jackson James M.^ORCID,Contreras Yanett^ORCID,Rathborne Jill M.^ORCID,Whitaker J. Scott^ORCID,Guzmán Andrés^ORCID,Stephens Ian W.^ORCID,Sanhueza Patricio^ORCID,Longmore Steven^ORCID,Zhang Qizhou^ORCID,Allingham David

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/869/i=2/a=102/pdf

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2. SIMULATIONS OF UNEQUAL BINARY COLLISIONS EMBEDDED IN A TURBULENT GAS CLOUD FAR FROM A MASSIVE GRAVITATIONAL CENTER;Revista Mexicana de Astronomía y Astrofísica;2022-10-01

3. The initial conditions for young massive cluster formation in the Galactic Centre: convergence of large-scale gas flows;Monthly Notices of the Royal Astronomical Society;2022-05-18

4. Empirical formulae to describe some physical properties of small groups of protogalaxies with multiplicity;Research in Astronomy and Astrophysics;2021-10-01

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