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Radio Core Size of Low-luminosity Active Galactic Nuclei under the Magnetically Arrested Disk–Jet Model

  • Authors: Yue Xu, 悦 许, Fu-Guo Xie, 富国 谢

Yue Xu et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

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.

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