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Radiation spectra of warm, optically thick coronae in AGNs · 2001 · DOI 10.1051/0004-6361/201937011

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astro-ph.HE 1

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2026 1

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A magnetically-supported disk-corona model for Changing-Look AGN transitions

astro-ph.HE · 2026-06-24 · unverdicted · novelty 7.0

Magnetized disk models lower the thermal-viscous instability threshold to Eddington ratios of 0.01-0.03 and yield limit-cycle timescales of months to years, jointly matching observations in five CLAGN only when the inner disk is strongly magnetized.

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  • A magnetically-supported disk-corona model for Changing-Look AGN transitions astro-ph.HE · 2026-06-24 · unverdicted · none · ref 59

    Magnetized disk models lower the thermal-viscous instability threshold to Eddington ratios of 0.01-0.03 and yield limit-cycle timescales of months to years, jointly matching observations in five CLAGN only when the inner disk is strongly magnetized.