Evolution of close-in Jupiter-mass planets around a 1.0 M_⊙ star of metallicity Z = 0.004 with an initial rotation period of 4.5 days. The colored solid lines correspond to the orbital period evolution of the planets. The colored dash-dotted lines correspond to the rotation period of the star and the colored dashed lines correspond to the 1 / 2 P_⋆ limit. The thick black dashed line corresponds to the Roche limit.