When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147
V. Silva Aguirre, K.R. Covey, S. Meibom, A.M. Cody et autres
Recent measurements of rotation periods () in the benchmark open clusters Praesepe (670 Myr), NGC 6811 (1 Gyr), and NGC 752 (1.4 Gyr) demonstrate that, after converging onto a tight sequence of slowly rotating stars in mass-period space, stars temporarily stop spinning …
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Carolina Digital Repository (University of North Carolina at Chapel Hill)