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 13.

Two instances of Hα profile asymmetries. The left panel depicts “LAMOST J121906.42+182120.7,” whereas the right panel shows “LAMOST J042836.05+082558.0.” In these panels, the red and green dashed lines denote the integration boundaries, the pink and blue dashed lines indicate the theoretical and actual peak positions of the Hα profile, and the bright blue and yellow lines emphasize the integration regions. For reference, the yellow dashed line presents the outcome of a double-Gaussian fit.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse