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. 19.

NGC 1068. Left half: high resolution HCO⁺(3−2) observations (Imanishi et al. 2020). Panel (a) moment 0 map (I₀ = 18420 K km s⁻¹), (b) moment 1 map (in km s⁻¹), (c) pv diagram along the major axis, and (d) pv diagram along the minor axis (T_b0 = 75 K). Right half: dense disk cloud model. Panel (e) moment 0 map, (f) moment 1 map (in km s⁻¹), (g) pv diagram along the major axis, and (h) pv diagram along the minor axis. The model levels are the same as those of the observed maps.

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