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Fig. 3.

image

Example simulation of rotation velocity according to the Bouvier et al. (1997) for a 1 M model. The black dot indicating the solar value at 4.5 Gyr. The input parameters are presented in Table 1. Shown are three different curves for different disk locking time, i.e. the time it takes the star to decouple from its surrounding protoplanetary disk.

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