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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 9.

The distribution of rotation-based stellar ages in the TESS SCVZ (the Gold sample in Table 1). The stars shown span an APOGEE temperature range of 3600–6100 K. We separate stars with periods less than 10 days, which are more likely to be tidally synchronized binaries than true rapid rotators (Simonian et al. 2019).

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