Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Recent radiation-thermochemical-magnetohydrodynamic simulations resolved formation of quasar accretion disks from cosmological scales down to ~300 gravitational radii $R_{g}$, arguing they were 'hyper-magnetized' (plasma $\beta\ll1$ supported by toroidal magnetic fields) and distinct from...

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Bibliographic Details
Main Authors: Philip F. Hopkins, Kung-Yi Su, Norman Murray, Ulrich P. Steinwandel, Nicholas Kaaz, Sam B. Ponnada, Jaeden Bardati, Joanna M. Piotrowska, Hai-Yang Wang, Yanlong Shi, Daniel Angles-Alcazar, Elias R. Most, Kyle Kremer, Claude-Andre Faucher-Giguere, Sarah Wellons
Format: Article
Language:English
Published: Maynooth Academic Publishing 2025-04-01
Series:The Open Journal of Astrophysics
Online Access:https://doi.org/10.33232/001c.137296
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