GMC Collisions as Triggers of Star Formation. II. 3D Turbulent, Magnetized Simulations

Wu, B, Tan, JC, Nakamura, F et al. (3 more authors) (2017) GMC Collisions as Triggers of Star Formation. II. 3D Turbulent, Magnetized Simulations. Astrophysical Journal, 835 (2). 137. pp. 1-23. ISSN 0004-637X

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2017, The American Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: ISM: clouds; ISM: kinematics and dynamics; ISM: lines and bands; ISM: magnetic fields; ISM: structure; methods: numerical
Dates:
  • Published: 23 January 2017
  • Accepted: 14 November 2016
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 23 Nov 2016 15:32
Last Modified: 18 Jul 2017 16:15
Published Version: https://doi.org/10.3847/1538-4357/835/2/137
Status: Published
Publisher: American Astronomical Society
Identification Number: https://doi.org/10.3847/1538-4357/835/2/137

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