Tidal dissipation in rotating and evolving giant planets with application to exoplanet systems

Lazovik, Y.A., Barker, A.J. orcid.org/0000-0003-4397-7332, de Vries, N.B. et al. (1 more author) (2024) Tidal dissipation in rotating and evolving giant planets with application to exoplanet systems. Monthly Notices of the Royal Astronomical Society, 527 (3). pp. 8245-8256. ISSN 0035-8711

Abstract

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Item Type: Article
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© 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

Keywords: planet-star interactions, planetary systems, planets and satellites, interiors, planets and satellites, physical evolution
Dates:
  • Published: January 2024
  • Published (online): 28 November 2023
  • Accepted: 27 November 2023
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:
Funder
Grant number
STFC (Science and Technology Facilities Council)
ST/W000873/1
STFC (Science and Technology Facilities Council)
ST/S000275/1
Depositing User: Symplectic Publications
Date Deposited: 28 Nov 2023 15:57
Last Modified: 19 Dec 2023 17:06
Status: Published
Publisher: Oxford University Press
Identification Number: 10.1093/mnras/stad3689
Open Archives Initiative ID (OAI ID):

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