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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 7.

Distributions of TESS flare duration and amplitude for RS CVn systems and other main-sequence eruptive stars. The left panels show the distributions of log Dur, where Dur is in hours, and the right panels show the distributions of log Amp. The histograms are normalized to percentage within each subsample.

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