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What drives the evolution of gas kinematics in star-forming galaxies?
External Source
chorus
Document Type
Version of Record
Authors
Chao-Ling Hung (Physics Department, Manhattan College, 4513 Manhattan College Pkwy, Bronx, NY 10471, USA)
Christopher C Hayward (Center for Computational Astrophysics, Flatiron Institute, 162 Fifth Avenue, New York, NY 10010, USA)
Tiantian Yuan (Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia)
Michael Boylan-Kolchin (Department of Astronomy, The University of Texas at Austin, Austin, TX 78712, USA)
Claude-André Faucher-Giguère (Department of Physics and Astronomy and CIERA, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208, USA)
Philip F Hopkins (TAPIR, Mailcode 350-17, California Institute of Technology, Pasadena, CA 91125, USA)
Dušan Kereš (Department of Physics, Center for Astrophysics and Space Sciences, University of California at San Diego, La Jolla, CA 92093, USA)
Norman Murray (Canadian Institute for Theoretical Astrophysics, 60 St George Street, University of Toronto, ON M5S 3H8, Canada)
Andrew Wetzel (Department of Physics, University of California, Davis, CA 95616, USA)
Date Acquired
June 7, 2025
Publication Date
March 11, 2018
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 482
Issue: 4
Issue Publication Date: January 2, 2019
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/sty2970
Funding Number(s)
funding: AST-1412836
funding: NNX15AB22G
Distribution Limits
Public

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