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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 9.

Radio size of MAD in LLAGNs. Here we take cases of ﹩{\dot{m}}_{0}=1\times 1{0}^{-4}﹩ (see light-green curves in the left panel for the SED) for illustration. Blue and red filled squares represent the radio size of MAD with ξpl,mad = 0 and ξpl,mad = 1% (cooling included), respectively. We emphasize that the radio size of LLAGNs at low frequency should be dominated by the jet component (if it exists).

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