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Rotation of Late-type Stars in Praesepe with K2

  • Authors: L. M. Rebull, J. R. Stauffer, L. A. Hillenbrand, A. M. Cody, J. Bouvier, D. R. Soderblom, M. Pinsonneault, and L. Hebb

2017 The Astrophysical Journal 839 92.

  • Provider: AAS Journals

Caption: Figure 1.

All 984 members or candidate members (see Section 2.5.4) of Praesepe with K2 LCs projected onto the sky. Note the gaps between K2 detectors. Stars that are >5° from the cluster center are highlighted in Appendix H.

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