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Fig. 2

image

Possible rotational evolution tracks of Proxima Cen (1 Ω = 2.67 × 10−6 rad s−1). The black star shows the modern observed rotation rate of Proxima Cen, which corresponds to a rotation period of ~ 82.5 days. The triangles indicate the observational constraints on the 10th and 90th percentiles of the rotational distributions from Irwin et al. (2011). The purple line corresponds to the evolution track of a fast rotator, the green line shows the evolution track of a slow rotator. All values in between are also possible.

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