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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Table 4.

Integrated intensities in Jy km s⁻¹ of the observations and the dense disk cloud model.

Line	I_obs	I_model
CO(2−1)	1.6	1.2
CO(3−2)	5.3	7.2
CO(6−5)	31.3	55.4
HCN(3−2)	2.5	2.7
HCN(4−3)	5.3	5.4
HCO⁺(3−2)	0.8	0.6
HCO⁺(4−3)	3.0	1.0 ^(a)
CS(7−6)	0.35	0.09 ^(b)

Notes.

^(a)

The intercloud gas model (Sect. 4.2.3) yields I_model = 2.0 Jy km s⁻¹.

^(b)

The intercloud gas model (Sect. 4.2.3) yields I_model = 0.26 Jy km s⁻¹. IR pumping is assumed for the HCN and HCO⁺ lines.

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