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. 1.

Fraction of dissipated energy per cloud-cloud collision as a function of the distance to the central black hole. The dissipation energy fraction is shown for all clouds during the NGC 1068 model evolution presented in Fig. 3.

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