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. 10.

CS(7−6) integrated intensity map. Upper panel: model. The contour levels are in steps of 22 K km s⁻¹ from 11 to 275 K km s⁻¹. The spatial resolution is 4.5″ × 3.1″. Lower panel: observations from Montero-Castaño et al. (2009). The rms is 2.5 K km s⁻¹. The contour levels are in steps of 15 K km s⁻¹ from 7 to 170 K km s⁻¹, but for the highest contour level at 190 K km s⁻¹. Sgr A^* is marked with a star.

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