Image Details

Choose export citation format:

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 3.

Distribution of flare events across different temperatures, masses, and spectral types. The top panels present histograms of the number of flares for stars with different effective temperatures (Teff), masses, and spectral types. The middle panels illustrate the proportion of flare stars across these same parameters. The bottom panels presents a comparison between our results and those of Z. Yang et al. (2023); the red bars represent our results, while the blue bars correspond to the results of Z. Yang et al. (2023).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse