On turbulence driven by axial precession and tidal evolution of the spin–orbit angle of close-in giant planets

Barker, AJ (2016) On turbulence driven by axial precession and tidal evolution of the spin–orbit angle of close-in giant planets. Monthly Notices of the Royal Astronomical Society, 460 (3). pp. 2339-2350. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • Barker, AJ
Copyright, Publisher and Additional Information: © 2016 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. This article has published in Monthly Notices of the Royal Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: instabilities; MHD; waves; planet; star interactions; binaries: close; planetary systems
Dates:
  • Published: 11 August 2016
  • Accepted: 12 May 2016
  • Published (online): 16 May 2016
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Funding Information:
FunderGrant number
Leverhulme TrustECF-2014-216
Depositing User: Symplectic Publications
Date Deposited: 02 Dec 2016 11:08
Last Modified: 02 Dec 2016 11:08
Published Version: https://doi.org/10.1093/mnras/stw1172
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stw1172

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