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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 8.

Two-dimensional density distributions of flare duration and bolometric flare energy for other main-sequence eruptive stars and RS CVn systems. The panels show log(Duration [min]) versus ﹩\mathrm{log}\left({E}_{\,{\rm{flare}}\,}[{\rm{erg}}]\right)﹩ for all available events and for the main temperature-defined spectral subclasses. Color represents the number of events per bin.

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