\begin{table}%t6 %\centering \par \caption{\label{predictions_HIFI}Predictions of the line fluxes (after subtraction of the continuum) of the water lines observable with the Herschel spectrometer HIFI.} \begin{tabular}{cccc} \hline \hline\noalign{\smallskip} HIFI range & & $X_{\rm in}$(H$_2$O) = $2\times10^{-6}$ & $X_{\rm in}$(H$_2$O) = $5\times10^{-8}$ \\ \hline Transition & Frequency & Flux & Flux \\ & (GHz) & (K Km s$^{-1}$) & (K Km s$^{-1}$) \\ \hline 1$_{ 1 0} \rightarrow $ 1$_{ 0 1}$ & 557.0 & 32 & 32 \\ 5$_{ 3 2} \rightarrow $ 4$_{ 4 1}$ & 620.7 & 0.31 & 0 \\ 2$_{ 1 1} \rightarrow $ 2$_{ 0 2}$ & 752.0 & 23 & 23 \\ 4$_{ 2 2} \rightarrow $ 3$_{ 3 1}$ & 916.2 & 0.04 & 0.04 \\ 2$_{ 0 2} \rightarrow $ 1$_{ 1 1}$ & 987.9 & 37 & 37 \\ 3$_{ 1 2} \rightarrow $ 3$_{ 0 3}$ & 1097.3 & 26 & 26 \\ 1$_{ 1 1} \rightarrow $ 0$_{ 0 0}$ & 1113.4 & 46 & 46 \\ 7$_{ 2 5} \rightarrow $ 8$_{ 1 8}$ & 1146.6 & 0.04 & 0 \\ 3$_{ 1 2} \rightarrow $ 2$_{ 2 1}$ & 1153.1 & 34 & 34 \\ 6$_{ 3 4} \rightarrow $ 5$_{ 4 1}$ & 1158.3 & 1.0 & 0 \\ 3$_{ 2 1} \rightarrow $ 3$_{ 1 2}$ & 1162.9 & 13 & 11 \\ 4$_{ 2 2} \rightarrow $ 4$_{ 1 3}$ & 1207.6 & 1.1 & 1.1 \\ 2$_{ 2 0} \rightarrow $ 2$_{ 1 1}$ & 1228.8 & 7.6 & 7.6 \\ 5$_{ 2 3} \rightarrow $ 5$_{ 1 4}$ & 1410.7 & 5.7 & 2.1 \\ 6$_{ 4 3} \rightarrow $ 7$_{ 1 6}$ & 1574.2 & 0.10 & 0 \\ 4$_{ 1 3} \rightarrow $ 4$_{ 0 4}$ & 1602.2 & 2.2 & 2.2 \\ 2$_{ 2 1} \rightarrow $ 2$_{ 1 2}$ & 1661.0 & 40 & 37 \\ 2$_{ 1 2} \rightarrow $ 1$_{ 0 1}$ & 1669.9 & 66 & 67 \\ 4$_{ 3 2} \rightarrow $ 5$_{ 0 5}$ & 1713.9 & 2.1 & 0.1 \\ 3$_{ 0 3} \rightarrow $ 2$_{ 1 2}$ & 1716.8 & 56 & 56 \\ 7$_{ 3 4} \rightarrow $ 7$_{ 2 5}$ & 1797.2 & 2.2 & 0.1 \\ 5$_{ 3 2} \rightarrow $ 5$_{ 2 3}$ & 1867.7 & 4.6 & 0.9 \\ 6$_{ 3 4} \rightarrow $ 7$_{ 0 7}$ & 1880.8 & 0.41 & 0 \\ 8$_{ 4 5} \rightarrow $ 7$_{ 5 2}$ & 1884.9 & 0.09 & 0 \\ 3$_{ 3 1} \rightarrow $ 4$_{ 0 4}$ & 1893.7 & 0.02 & 0.02 \\ & & & \\ \hline \end{tabular} \tablefoot{The third (fourth) column reports the predictions computed assuming that the inner H$_2$O abundance is equal to $2\times10^{-6}$ ($5\times10^{-8}$) and the outer H$_2$O abundance is $2.5\times10^{-7}$, for the Shu-like model best-fit.} \end{table}