A QPO candidate in NGC 1566 supports misaligned accretion flows fueled by captured broad-line region clouds as the cause of rapid changing-look AGN transitions.
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Upper limits on the shortest AGN variability timescales are log(t_min,ul/hrs) = 0.85 ± 0.55, interpreted as light-crossing times from a few to thousands of gravitational radii in regions smaller than accretion disks.
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X-ray Quasi-Periodic Oscillations in Active Galactic Nuclei and Their Implications for the Changing Look Phenomenon
A QPO candidate in NGC 1566 supports misaligned accretion flows fueled by captured broad-line region clouds as the cause of rapid changing-look AGN transitions.
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The shortest detected intra-day variability of active galactic nuclei in TESS survey
Upper limits on the shortest AGN variability timescales are log(t_min,ul/hrs) = 0.85 ± 0.55, interpreted as light-crossing times from a few to thousands of gravitational radii in regions smaller than accretion disks.