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Fig. 10.

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Ratio of the complex parts of the Love number for the dynamical to equilibrium tide (Im(k22)IGW/Im(k22)eq) as a function of the orbital period and stellar age for a MZAMS = 1 M star. The critical period, Pc, above which companions excite progressive IGWs, is shown in orange. R (in brown) represents the orbital period on which a planet orbits at the surface of the star, and the Roche limit is given in purple. Changes in the stellar evolutionary phase are indicated with ticks on the upper axis.

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