From the Circumnuclear Disk in the Galactic Center to thick, obscuring tori of AGNs - Modeling the molecular emission of a parsec-scale torus as found in NGC 1068

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Fig. 14.

Model mass accretion rate measured at R = 0.25 pc. Solid line: preferred model with ξ = 0.9, dashed line: preferred model without the massive infalling gas cloud, vertical line: time of interest.

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