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Fig. 5

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a)F6/F4 (oH2O 321−312-to-pH2O 220−211) and b) F6/F2 (oH2O 321−312-to-pH2O 202−111) line flux ratios as a function of the 75-to-100 μm far-IR color. Blue symbols: NH2OV = 1015cm-2/ (km s-1) and τ100 ≤ 0.1; black: NH2OV = 5 × 1015cm-2/ (km s-1) and τ100 ≤ 0.1; red: NH2OV = 5 × 1015cm-2/ (km s-1) and τ100 = 1.0; green: NH2OV = 1015cm-2/ (km s-1) and τ100 = 1.0; magenta: same as blue symbols but with collisional excitation included with Tgas = 150 K and nH2 = 3 × 105 cm-3. The small numbers close to the symbols indicate the value of Tdust . The observed averaged ratios for strong-AGN and HII+mild-AGN sources (Y13) are indicated with dashed horizontal lines, and indicate that the regions probed by the H2O submm emission are characterized by warm dust (Tdust ≳ 45 K).

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