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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 6.

Toroidal magnetic field weighted by ﹩{(r/{r}_{{\rm{g}}})}^{1/2}﹩ in run HS at time t = 110,700 rg/c. The toroidal field is roughly symmetric (antisymmetric) about the midplane beyond (within) ≈200 rg. (a) Equatorial snapshot of the toroidal field within ≈500 rg. Magnetic field lines are shown in black. (b) Same as panel (a), except we show the x − z plane.

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