Fig. 5
Top: evolution of the semi-major axis (full lines) of a close-in Jupiter-mass planet around initially fast-rotating 1 M⊙ stars of different metallicities: Z = 0.004 in dark-blue, Z = 0.0134 in cyan and Z = 0.0255 in pink. The dash-dotted lines correspond to the corotation radius. The colored dotted lines correspond to the radius of the star and the black dashed line corresponds to the Roche limit. Bottom: evolution of the dissipation factor of the different 1 M⊙ stars.
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