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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 3.

The time evolution of MAD parameters Φ B . The left column represents retrograde disks, while the right column is for prograde disks. We use the horizontal lines to denote the time-averaged Φ B from 104 t g to 2 × 104 t g , which is referred to as the typical MAD parameter during the MAD state.

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