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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 10.

Time and azimuthally averaged density ρ, ratio of gas to magnetic pressure β, and magnetization σ for aM94b100 (top), a0b100 (middle), and a94b100 (bottom). The black lines in the middle and right panels represent the β = 1 and σ = 1 conditions, respectively. The white wedges at the poles correspond to the first cell close to the pole.

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