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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 2.

Normalized response function ﹩{\bar{F}}_{{\ell },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 real (imaginary) part of the function is shown in the upper (lower) panel, and separate curves are plotted for the DS and MD approaches. Peaks are labeled by the resonant mode's classification within the Eckart–Osaki–Scuflaire scheme. The upper axis scale shows the tidal forcing angular frequency σ m,k (Equation (7)).

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