Multi-wavelength Emission Modeling from Accretion Flows around Isolated Black Holes Including Magnetic Flux Transport

arXiv:2606.31477 · astro-ph.HE · Submitted 2026-06-30 · Read on arXiv

astro-ph.HE

Submitted: 2026-06-30

Updated: 2026-09-19

Comments: 16 pages, 10 figures. Submitted to The Astrophysical Journal

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Accretion Flows — 6× in this paper · explained in 1 episode
• AGN — 4× in this paper · explained in 1 episode
• Core — 2× in this paper · explained in 2 episodes
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Ambipolar Diffusion — 1× in this paper · explained in 1 episode
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Microlensing — 1× in this paper · explained in 2 episodes

Sources

• Demystifying flux eruptions: Magnetic flux transport in magnetically arrested disks

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