Fig. 8.
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Evolution of the fast rotator sequence in time. The highlighted sequences (from left to right) belong to NGC 3532 (300 Myr, orange triangles), NGC 2281 (430 Myr, black circles), M 37 (450 Myr, black squares), M 44 (Praesepe 670 Myr, blue stars). The large errorbars indicate the positions and ranges of rotation periods used in the text to estimate the spin-down rate. Grey symbols in the background denote other rotators in these open clusters and are marked with the respective symbols.
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