Tidal dissipation in evolving low-mass and solar-type stars with predictions for planetary orbital decay

Barker, A orcid.org/0000-0003-4397-7332 (2020) Tidal dissipation in evolving low-mass and solar-type stars with predictions for planetary orbital decay. Monthly Notices of the Royal Astronomical Society, 498 (2). pp. 2270-2294. ISSN 0035-8711

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Authors/Creators:
Copyright, Publisher and Additional Information: © The Author(s) 2020. 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: planet-star interactions; planetary systems; binaries: close; stars: rotation; stars: interiors; stars: solar-type
Dates:
  • Accepted: 6 August 2020
  • Published (online): 2 September 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: 10 Aug 2020 12:24
Last Modified: 06 Dec 2020 18:50
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/staa2405

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