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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 8.

Spacetime (﹩{\rm{log}}r-t﹩) diagram of the magnetic field parity (C(UDUQ); see Equations (19)–(20) in runs HS (panel (a)) and NS (panel (b)), where 1, −1, and 0 indicate dipole-like/odd parity, quadrupole-like/even parity, and mixed parity, respectively. By late times, the disk is odd at r ≲ 200 rg and even at larger radii in both runs. We have also marked the time when our radiation module is activated with a black line.

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