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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 5.

The long-time evolution of the mass accretion rate and MAD parameters for simulation aM94b100h. The MAD parameter remains steady with time, although the mass accretion drops.

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