Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries

Barker, AJ orcid.org/0000-0003-4397-7332 (2022) Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries. Astrophysical Journal Letters, 927 (2). L36. ISSN 2041-8205

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2022. The Author(s). This is an open access article under the terms of the Creative Commons Attribution 4.0 International License (CC BY 4.0) (https://creativecommons.org/licenses/by/4.0/)
Dates:
  • Accepted: 7 March 2022
  • Published (online): 17 March 2022
  • Published: 17 March 2022
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: 09 Mar 2022 16:09
Last Modified: 23 May 2022 11:28
Status: Published
Publisher: IOP Publishing
Identification Number: https://doi.org/10.3847/2041-8213/ac5b63

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