Open Access

Fig. C.4

image

Secular evolution of a star–planet system composed by a 1 M star and a 1 MJup planet with an initial stellar rotation period P*,ini = 5 days and an initial semi-major axis aini = 0.025 AU. Red curves were computed for ω1 = 10−10 rad/s and blue curves, for ω1 = 10−6 rad/s. Top panel: semi-major axis (solid lines), stellar corotation radius (dashed lines), limit of excitation of tidal inertial waves (dotted lines), stellar radius (solid black line) and Roche limit (dashed gray line). Bottom panel: modified tidal quality factor.

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