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TESS Stellar Rotation up to 80 Days in the Southern Continuous Viewing Zone

  • Authors: Zachary R. Claytor, Jennifer L. van Saders, Lyra Cao, Marc H. Pinsonneault, Johanna Teske, Rachael L. Beaton

Zachary R. Claytor et al 2024 The Astrophysical Journal 962 .

  • Provider: AAS Journals

Caption: Figure 14.

The detectability of rotation across APOGEE metallicity and α-element abundace. The color bar corresponding to the detection fraction has a maximum value of 50%. We detect fewer stars in rotation at high [α/M] because these stars tend to be old, slowly rotating, and less active. At fixed [α/M], there is scatter in the trend of detectability with metallicity from bin to bin.

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