Efficiency of tidal dissipation in slowly rotating fully convective stars or planets

Vidal, J orcid.org/0000-0002-3654-6633 and Barker, AJ orcid.org/0000-0003-4397-7332 (2020) Efficiency of tidal dissipation in slowly rotating fully convective stars or planets. Monthly Notices of the Royal Astronomical Society, 497 (4). pp. 4472-4485. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This is an author produced version of an article published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: convection, hydrodynamics, planet–star interactions, binaries: close
Dates:
  • Accepted: 23 July 2020
  • Published (online): 6 August 2020
  • Published: October 2020
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Funding Information:
FunderGrant number
STFC (Science and Technology Facilities Council)ST/R00059X/1
STFC (Science and Technology Facilities Council)ST/S000275/1
Depositing User: Symplectic Publications
Date Deposited: 30 Jul 2020 16:02
Last Modified: 04 Sep 2020 12:59
Status: Published
Publisher: Oxford University Press (OUP)
Identification Number: https://doi.org/10.1093/mnras/staa2239

Share / Export

Statistics