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Discrepant Approaches to Modeling Stellar Tides and the Blurring of Pseudosynchronization

  • Authors: R. H. D. Townsend, M. Sun, 萌 孙

R. H. D. Townsend et al 2023 The Astrophysical Journal 953 .

  • Provider: AAS Journals

Caption: Figure 3.

Damping coefficient γ ,m,k plotted against stellar rotation frequency f rot for the {, m, k} = {2, −2, 50} partial tide of the KOI-54 primary model. The dashed vertical lines correspond to the resonances shown in Figure 2. The upper axis scale shows the tidal forcing angular frequency σ m,k (Equation (7)).

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