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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 17.

The relationship between ﹩\mathrm{log}({F}_{{\rm{X}}}/{F}_{\mathrm{bol}})﹩ and BP – RP. The color bar shows ﹩\mathrm{log}({\rm{Distance}})﹩. Hollow triangles with black edges denote stars without flares, while hollow circles with red edges denote stars with flares. The upper panels correspond to the low-resolution data, and the lower panels correspond to the medium-resolution data.

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