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Fig. 5.


Top: evolution of the semi-major axis (dashed line) and the rotation velocity (solid line) of a 0.8 M star with [Fe/H] = − 0.4 and a 10 MJup companion at a distance of a0 = 0.02 AU. Bottom: same conditions for the same stellar model with a 10 MJup companion at a0 = 0.03 AU. No engulfment occurs during the MS lifetime.

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