Disk Structure May Determine AGN Variability and Explain the Accretion Disk Size Problem: No Broad Line Region Required
astro-ph.HE, astro-ph.GA
Submitted: 2026-10-08
Updated: 2026-10-08
Terminology
Sources
- Testing disc reprocessing models for AGN optical variability by comparison of X-ray and optical power spectra of NGC 4395
- Amoeba: An AGN Model of Optical Emissions Beyond steady-state Accretion discs
- Frequency-resolved lags in UV/optical continuum reverberation mapping
- AGN STORM 2. IV. Swift X-ray and ultraviolet/optical monitoring of Mrk 817
- AGN Continuum Reverberation Mapping Based on Zwicky Transient Facility Light Curves
- FORGE'd in FIRE II: The Formation of Magnetically-Dominated Quasar Accretion Disks from Cosmological Initial Conditions
- Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum
- Magnetosonic Waves as a Driver of Observed Temperature Fluctuation Patterns in AGN Accretion Disks
- AGN STORM 2. XII. Ground-Based Optical Photometry and Lag Measurements of Mrk 817
- AGN STORM 2. VI. Mapping Temperature Fluctuations in the Accretion Disk of Mrk 817
- Negative Lags on the Viscous Timescale in Quasar Photometry and Prospects for Detecting More with LSST
- Measuring the Vertical Structure of Active Galactic Nuclei Disks with Transformer Models and the Vera C. Rubin Observatory
- Continuum Reverberation in Bright Quasars Using NASA/ATLAS
- A Negative Long Lag from the Optical to the UV Continuum in Fairall 9
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