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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 1.

The distribution of flare duration and amplitude. The upper left panel shows a statistical histogram of flare durations, with the upper right panel presenting a histogram of flare amplitudes. Subplots offer a detailed view of durations exceeding 2.0 and amplitudes exceeding 0.2, while the lower panels depict the proportion of flare durations and amplitudes in each interval after logarithmic transformation.

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