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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 9.

Empirical duration–energy relations for TESS flares in other MS eruptive stars and RS CVn systems. The two samples are displayed in separate full-width halves of the figure. Individual flare measurements are color coded by effective temperature. Red lines show the fitted relations in the log (Duration [min])– ﹩\mathrm{log}\left({E}_{\,{\rm{flare}}\,}\right.﹩ [erg]) plane, and the shaded regions show the 1σ and 3σ scatter ranges. The fitted slopes and Spearman statistics are listed in each panel.

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