The evolution of binary populations in cool, clumpy star clusters

Parker, R.J., Goodwin, S.P. and Allison, R.J. (2011) The evolution of binary populations in cool, clumpy star clusters. Monthly Notices of the Royal Astronomical Society, 418 (4). pp. 2565-2575. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • Parker, R.J.
  • Goodwin, S.P.
  • Allison, R.J.
Copyright, Publisher and Additional Information: © 2011 The Authors © 2011 RAS. This is an author produced version of a paper subsequently published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: methods: numerical; stars: formation; Galaxy: kinematics and dynamics; open clusters and associations: general
Dates:
  • Published: 21 December 2011
  • Accepted: 17 August 2011
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 17 Aug 2017 12:12
Last Modified: 22 Mar 2018 00:42
Published Version: https://doi.org/10.1111/j.1365-2966.2011.19646.x
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1111/j.1365-2966.2011.19646.x
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