Spin dynamics of close-in planets exhibiting large transit timing variations

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Fig. 5

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Examples of the spin evolution of Kepler-88 b and corresponding global C₂₂ value for different τ values. We use the initial conditions from Table 3, and the initial rotation period is set at 10 d. The green lines give the position of the spin-orbit resonances n, n ± ν/ 2, and n ± ν.

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