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