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Why Are Rapidly Rotating M Dwarfs in the Pleiades so (Infra)red? New Period Measurements Confirm Rotation-dependent Color Offsets From the Cluster Sequence

MPS-Authors

Covey,  K.R.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Agüeros,  M.A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Law,  N.M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Liu,  J.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Ahmadi,  A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Laher,  R.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Levitan,  D.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Sesar,  B.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Surace, 
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Citation

Covey, K., Agüeros, M., Law, N., Liu, J., Ahmadi, A., Laher, R., et al. (2016). Why Are Rapidly Rotating M Dwarfs in the Pleiades so (Infra)red? New Period Measurements Confirm Rotation-dependent Color Offsets From the Cluster Sequence. Astrophysical Journal, 822: 81, pp. 81. doi:10.3847/0004-637X/822/2/81.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002E-15C8-D
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