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Stellar Parameters and Magnetic Activity of Eruptive Variable Stars Based on TESS Light Curves and the LAMOST Spectral Survey

  • Authors: Yanan Wang, Li-yun Zhang, Tianhao Su, Xianming L. Han, Prabhakar Misra

Yanan Wang et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 5.

Relationship between source-level log ﹩R{{\prime} }_{{\rm{H}}\alpha }﹩ and multiepoch Hα equivalent-width variability. Other MS eruptive stars and RS CVn systems are shown separately. The left panels show the absolute scatter σ(∣EWHα∣), and the right panels show the relative scatter σ(∣EWHα∣)/〈∣EWHα∣〉. The vertical-axis quantities are calculated from the magnitude of the directly measured multiepoch equivalent widths, whereas the horizontal coordinate is the source-level-normalized excess-emission index. Red connected points show binned medians, and the Spearman coefficients and p-values are listed in each panel.

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