A hybrid SPH/N-body method for star cluster simulations

Hubber, D.A., Allison, R.J., Smith, R. et al. (1 more author) (2013) A hybrid SPH/N-body method for star cluster simulations. Monthly Notices of the Royal Astronomical Society, 430 (3). pp. 1599-1616. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • Hubber, D.A.
  • Allison, R.J.
  • Smith, R.
  • Goodwin, S.P.
Copyright, Publisher and Additional Information: This article has been accepted for publication in MNRAS ©: 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: hydrodynamics; methods: numerical; stars: kinematics and dynamics
Dates:
  • Published: April 2013
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: 03 Nov 2017 14:50
Last Modified: 03 Nov 2017 14:50
Published Version: https://doi.org/10.1093/mnras/sts694
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1093/mnras/sts694
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