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Predictions for the spatial distribution of the dust continuum emission in $\boldsymbol {1\,\lt\, z\,\lt\, 5}$ star-forming galaxies
External Source
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Document Type
Version of Record
Authors
R K Cochrane (SUPA, Institute for Astronomy, Royal Observatory, Edinburgh EH9 3HJ, UK)
C C Hayward (Center for Computational Astrophysics, Flatiron Institute, 162 Fifth Avenue, New York, NY 10010, USA)
D Anglés-Alcázar (Center for Computational Astrophysics, Flatiron Institute, 162 Fifth Avenue, New York, NY 10010, USA)
J Lotz (Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA)
T Parsotan (Department of Physics, Oregon State University, 301 Weniger Hall, Corvallis, OR 97331, USA)
X Ma (Department of Astronomy and Theoretical Astrophysics Center, University of California Berkeley, Berkeley, CA 94720, USA)
D Kereš (Department of Physics, Center for Astrophysics and Space Sciences, University of California, San Diego, La Jolla, CA, USA)
R Feldmann (Institute for Computational Science, University of Zurich, Zurich CH- 8057, Switzerland)
C A Faucher-Giguère (Department of Physics and Astronomy and CIERA, Northwestern University, Evanston, IL 60208, USA)
P F Hopkins (TAPIR, MC 350-17, California Institute of Technology, Pasadena, CA 91125, USA)
Date Acquired
February 10, 2024
Publication Date
June 25, 2019
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 488
Issue: 2
Issue Publication Date: September 11, 2019
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/stz1736
Funding Number(s)
funding: AST-1715101
funding: 157591
funding: 17-ATP17-0067
funding: HST-AR-14562.001
Distribution Limits
Public
Keywords
space and planetary science
astronomy and astrophysics

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