The split main sequence in the open cluster NGC 2287 is caused by a bimodal distribution of stellar rotation rates, with blue stars rotating near 100 km/s and red stars near 280 km/s.
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Tidal-locking-induced stellar rotation dichotomy in the open cluster NGC 2287?
The split main sequence in the open cluster NGC 2287 is caused by a bimodal distribution of stellar rotation rates, with blue stars rotating near 100 km/s and red stars near 280 km/s.