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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2 Pith papers cite this work. Polarity classification is still indexing.
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Type-C QPOs in MAXI J1348-630 exhibit stable ~7 Hz frequency despite intensity changes, hard rms spectra with peaks above 20 keV, and opposite hysteresis in frequency-flux relations between main and mini-outbursts.
citing papers explorer
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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 full evolution of the type-C QPO in MAXI J1348-630 revealed by Insight-HXMT
Type-C QPOs in MAXI J1348-630 exhibit stable ~7 Hz frequency despite intensity changes, hard rms spectra with peaks above 20 keV, and opposite hysteresis in frequency-flux relations between main and mini-outbursts.