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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 15.

Distribution of the cumulative TESS observing time for stars in our sample. The histograms show the number of stars in each 20 day bin for flare stars (orange) and nonflare stars (blue). The overplotted lines represent the fractions of flare and nonflare stars as a function of cumulative observing time.

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