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A Study of the Accretion State of Magnetically Arrested Disks across Black Hole Spins for Radiatively Inefficient Accretion Flows

  • Authors: G.-Q. Zhang, Damien Bégué, A. Pe'er, B.-B. Zhang

G.-Q. Zhang et al 2024 The Astrophysical Journal 962 .

  • Provider: AAS Journals

Caption: Figure 15.

Toroidal component of the four-velocity u ϕ and b r b ϕ as a function of θ for a94b100 (top), a0b100 (middle), and aM94b100 (bottom) at the radii at which the radial angular momentum flux is obtained.

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