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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 9.

Distribution of ﹩(V-{K}_{{\rm{s}}})﹩ values for the member sample with rotation periods in both Praesepe (solid line) and the Pleiades (dotted line). The y-axis is in units of sample fraction. We are sampling the same range of ﹩(V-{K}_{{\rm{s}}})﹩ values overall in the two clusters; there are notable differences at the bluest and reddest ends.

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