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. 22.

NGC 1068 intercloud gas model. Characteristics of individual model intercloud gas across the disk at the time of interest. Q = 30, ζ_CR = 2 × 10⁻¹³ s⁻¹, and full turbulent heating. Gas cloud characteristics. From upper left to lower right: cloud mass, size, density, H₂ column density, gas and dust temperatures, optical depth, and brightness temperature.

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