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H-AMR FORGE’d in FIRE. I. Magnetic State Transitions, Jet Launching, and Radiative Emission in Super-Eddington, Highly Magnetized Quasar Disks Formed from Cosmological Initial Conditions

  • Authors: Nicholas Kaaz, Matthew Liska, Alexander Tchekhovskoy, Philip F. Hopkins, Jonatan Jacquemin-Ide

Nicholas Kaaz et al 2025 The Astrophysical Journal 979 .

  • Provider: AAS Journals

Caption: Figure 3.

Net toroidal (ΦT, Equation (5)) and vertical (ΦV, Equation (6)) magnetic flux as a function of radius at t = 110,700 rg/c. At r ≳ 200 rg, the disk is dominated by the net toroidal flux (NTF), and within it is dominated by the net vertical flux (NVF). So, we refer to these as the NTF and NVF regions, respectively.

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