In NGC 2287, blue main-sequence stars rotate slower on average than red main-sequence stars, and the distribution of rotation speeds is best fitted by two separate populations at roughly 100 and 280 km/s.
D., Broby Nielsen, P., Ferguson, A
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Stellar rotation bifurcation caused by tidal locking in the open cluster NGC 2287?
In NGC 2287, blue main-sequence stars rotate slower on average than red main-sequence stars, and the distribution of rotation speeds is best fitted by two separate populations at roughly 100 and 280 km/s.