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. C.1.

NGC 1068. Left panel: HCN(3−2) high resolution spectra along the major axis (from Impellizzeri et al. 2019 data). Right panel: high-resolution HCN(3−2) spectra along the major axis of the dense disk cloud model with IR pumping.

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