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A VLBA-resolved Jet Associated with Super-Eddington Accretion in a Radio-loud Quasar at z = 3.4

  • Authors: Sakiko Obuchi, Ingyin Zaw, Kazuhiro Hada, Kohei Ichikawa, Joseph D. Gelfand

Sakiko Obuchi et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 3.

Jet viewing angle ϕ versus intrinsic jet speed β. The blue solid curve shows the lower limit of the βϕ relation derived from the constraint J ≳ 2.92, and the other solid curves (red, orange, green, purple, and black) correspond to Doppler factors ranging from 1 to 10. The shaded region represents the allowed parameter space satisfying the constraints on ϕ and β, i.e., J ≳ 2.92 and δ ∼ 1 (δ < 2).

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