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The Solar-like Latitudinal Distribution of Flaring Activities Revealed by TESS, APOGEE, and GALAH

  • Authors: Huiqin Yang, Shuai Liu, Yang Huang, Bowen Zhang, Jifeng Liu

Huiqin Yang et al 2026 The Astrophysical Journal Supplement Series 283 .

  • Provider: AAS Journals

Caption: Figure 2.

The detection rates of flaring stars along with inclination in the C, g, and I phases. The detection rate is the ratio between the number of flaring stars and the number of rotating stars in a sini bin. Error bars of each sini bin were estimated using the square root of the number of flaring stars in each bin.

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