Fig. 9
As Fig. 5, but with 5 MJ planets. We can see that since the planet is more massive than in Fig. 5 the acceleration of the star is more visible. Some slow rotators even become fast rotators for a few 10 Myr because of the merger of the planet. When a merger occurs the star is spun up to a rotation rate, which is on the order of 20 Ω⊙.
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