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Fig. 18.

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NGC 1068. Left half: high resolution HCN(3−2) observations (Impellizzeri et al. 2019). Panel (a) moment 0 map (I0 = 17300 K km s−1), (b) pv diagram along the major axis, (c) pv diagram along the minor axis (Tb0 = 70 K), (d) moment 1 map (in km s−1), (e) continuum map (contour levels are (0.019, 0.037, 0.075, 0.15, 0.3, 0.6, 1, 2, 4, 8)×43 K). Right half: high resolution HCN(3−2) emission of the dense disk cloud model with IR pumping. Panel (f) moment 0 map, (g) pv diagram along the major axis, (h) pv diagram along the minor axis, (i) unsmoothed pv diagram along the major axis, (j) moment 1 map (in km s−1), (k) continuum map. The model levels are the same as those of the observed maps. The additional white contour is at 80 K.

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