The prevalence of star formation as a function of Galactocentric radius

Ragan, SE, Moore, TJT, Eden, DJ et al. (3 more authors) (2016) The prevalence of star formation as a function of Galactocentric radius. Monthly Notices of the Royal Astronomical Society, 462 (3). pp. 3123-3129. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • Ragan, SE
  • Moore, TJT
  • Eden, DJ
  • Hoare, MG
  • Elia, D
  • Molinari, S
Copyright, Publisher and Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2016 The Authors; Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: stars: formation; ISM: clouds; galaxies: ISM
Dates:
  • Published: 1 November 2016
  • Accepted: 26 July 2016
  • Published (online): 30 July 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: 17 Oct 2016 10:03
Last Modified: 17 Oct 2016 10:03
Published Version: https://dx.doi.org/10.1093/mnras/stw1870
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stw1870

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