Rotating thin rings of absorbing material above the inner accretion disk reproduce the observed blueshifted absorption forests in XRISM spectra of AGN such as PDS 456.
The Soft X-ray View of the Ultra Fast Outflow
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Variable column density and covering factor of three ionized absorbers in clumpy disk winds explain the X-ray variability in I Zw 1 with stable corona.
citing papers explorer
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Blueshifted lines from the inner accretion disc's rotation can explain quasar absorption "forests''
Rotating thin rings of absorbing material above the inner accretion disk reproduce the observed blueshifted absorption forests in XRISM spectra of AGN such as PDS 456.
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Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds
Variable column density and covering factor of three ionized absorbers in clumpy disk winds explain the X-ray variability in I Zw 1 with stable corona.