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- W2062608889 abstract "We argue that the X-ray and UV flux illuminating the parsec-scale accretion disk around luminous active galactic nuclei (AGNs) is super-Eddington with respect to the local far-infrared dust opacity. The far-infrared opacity may be larger than in the interstellar medium of the Milky Way due to a combination of supersolar metallicity and the growth of dust grains in the dense accretion disk. Because of the irradiating flux, the outer accretion disk puffs up with a vertical thickness h ~ R. This provides a mechanism for generating a geometrically thick obscuring region from an intrinsically thin disk. We find obscuring columns ~1022-1023 cm-2, in reasonable agreement with observations." @default.
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- W2062608889 date "2007-06-10" @default.
- W2062608889 modified "2023-10-01" @default.
- W2062608889 title "From Thin to Thick: The Impact of X‐Ray Irradiation on Accretion Disks in Active Galactic Nuclei" @default.
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- W2062608889 doi "https://doi.org/10.1086/517960" @default.
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