Image Details
Caption: Figure 10.
Broadband SED of MAD models under different setups of PL electrons. From top to bottom, lines with the same color represent MADs whose accretion rates are ﹩{\dot{m}}_{0}=1\times 1{0}^{-2}﹩, 1 × 10−3, 1 × 10−4, and 1 × 10−5, respectively. Solid and dashed lines are for cases that only include thermal electrons (ξpl,mad = 0) and self-consistently include ξpl,mad = 5% PL electrons, respectively.
© 2026. The Author(s). Published by the American Astronomical Society.