Image Details

Choose export citation format:

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 3.

Comparison of periods obtained here to periods obtained in the literature. First panel: Scholz et al. (2011, 40 stars in common); second panel: SuperWASP (Delorme et al. 2011, 39 stars in common); third panel: HATNet (Kovács et al. 2014, 151 stars in common); fourth panel: PTF (Agüeros et al. 2011, 29 stars in common). The gray lines are at 1-to-1, P/2, and 2P. Most of the periods match well (see the text).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse