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Magnetic Activity in X-Ray Stars from eROSITA: Insights from the TESS and LAMOST Surveys

  • Authors: Lulu Xu, Li-yun Zhang, Yinpeng Wang, Tianhao Su, Xianming L. Han, Adriana M. Pires, Rui Guo, Xian Zhang, Prabhakar Misra, Qingfeng Pi, Hongpeng Lu

Lulu Xu et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 5.

Flare occurrence percentages as a function of different stellar parameters. Left panel: effective temperature versus rotation period. Right panel: LX/Lbol versus effective temperature. In both panels, colors distinguish flare and nonflare stars, and marker sizes indicate the flare occurrence fractions.

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