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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 3.

Inclination sini vs. the flaring activity in different Ro bins. The size of the filled circles represents the flaring frequency of a star. The green dashed line represents the best match of the stellar LaDAR. The shaded region represents the uncertainty caused by the maximum and minimum of the solar cycle. The uncertainty of log﹩{R}_{{\rm{flare}}}﹩ is 0.26 dex, which is from the error propagation of the flare energy. The uncertainty of sini is from the 16th and 84th percentiles of the posterior probability distribution of sini.

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