Tidal dissipation and spin-orbit alignment due to the precessional instability in convection zones in rotating giant planets and stars

de Vries, N.B., Barker, A.J. orcid.org/0000-0003-4397-7332 and Hollerbach, R. (Accepted: 2025) Tidal dissipation and spin-orbit alignment due to the precessional instability in convection zones in rotating giant planets and stars. Monthly Notices of the Royal Astronomical Society. ISSN: 0035-8711 (In Press)

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Item Type: Article
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This is an author produced version of an article accepted for publication in Monthly Notices of the Royal Astronomical Society made available under the terms of the Creative Commons Attribution License (CC-BY), which permits unrestricted use, distribution and reproduction in any medium, provided the original work is properly cited.
Dates:
  • Accepted: 29 October 2025
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds)
Funding Information:
Funder
Grant number
STFC (Science and Technology Facilities Council)
ST/S000275/1
STFC (Science and Technology Facilities Council)
ST/W000873/1
STFC Polaris House
UKRI1179
Date Deposited: 30 Oct 2025 13:40
Last Modified: 30 Oct 2025 13:40
Status: In Press
Publisher: Oxford University Press
Open Archives Initiative ID (OAI ID):

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