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. 15.

NGC 1068 Q = 30 analytical model of a turbulent clumpy gas disk (Sect. 2.2). Characteristics of individual model disk gas clouds across the disk at the time of interest. From upper left to lower right: cloud mass, size, density, H₂ column density, gas and dust temperatures, optical depth, and brightness temperature. IR pumping is included for the HCN and HCO⁺ lines.

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