Can the stellar dynamical tide destabilize the resonant chains of planets formed in the disk?

Kwok, L.K.W., Bolmont, E., Revol, A. et al. (4 more authors) (2024) Can the stellar dynamical tide destabilize the resonant chains of planets formed in the disk? In: Proceedings of the International Astronomical Union. Complex Planetary Systems II – Kavli-IAU Symposium 382, 03-07 Jul 2023, Namur, Belgium. Cambridge University Press , pp. 146-148.

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Item Type: Proceedings Paper
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© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union. This is an Open Access article, distributed under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives licence (http://creativecommons.org/licenses/by-nc-nd/4.0/), which permits non-commercial re-use, distribution, and reproduction in any medium, provided that no alterations are made and the original article is properly cited. The written permission of Cambridge University Press must be obtained prior to any commercial use and/or adaptation of the article.

Keywords: star-planet interactions; planetary dynamics; mean motion resonances (MMRs); resonant chains; tidal interactions; stellar tides; dynamical tides
Dates:
  • Published: 16 October 2024
  • Published (online): 16 October 2024
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
Leverhulme Trust
ECF-2022-362
Depositing User: Symplectic Publications
Date Deposited: 23 Jan 2025 14:47
Last Modified: 23 Jan 2025 14:47
Status: Published
Publisher: Cambridge University Press
Identification Number: 10.1017/S1743921323004210
Open Archives Initiative ID (OAI ID):

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