Figure 16 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 16.

The distribution of spot filling fractions separated by whether rotation was detected in the Gaia color range 1.5 < G _BP − G _RP < 2. While we might expect more spotted stars to be easier to detect in rotation, there are too few stars to draw any statistically significant conclusions.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions