Image Details
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.
© 2026. The Author(s). Published by the American Astronomical Society.