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

Open Access

Fig. 27.

ALMA integrated spectra of the central source S1 of NGC 1068 (black line). Upper panel: HCN(4−3); middle panel: CN(3−2); lower panel: CS(7−6). The gray line corresponds to the second component of the CN(3−2) triplet. Colored lines: dashed: S1 spectrum from the dense disk cloud model; dotted: S1 spectrum from the diffuse gas model.

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