Image Details
Caption: Figure 5.
(a)–(b) Scatter plots between two B h -increase parameters and IRS. The solid curve in (a) represents an exponential fitting. The dashed line represents the linear fitting. “cc” indicates the correlation coefficient. (c)–(d) Scatter plots between the parameters and flare magnitude shown for comparison.
© 2022. The Author(s). Published by the American Astronomical Society.