\begin{table}%t6 \caption{\label{tab6}Model results.} \small%\centering \par \begin{tabular}{llllccc} \hline \hline\noalign{\smallskip} \multicolumn{1}{c}{Source} & \multicolumn{1}{c}{Model} & \multicolumn{1}{c}{CO~Binding energy} & \multicolumn{1}{c}{$\chi$$_{\rm C^{18}O}$\tablefootmark{a}} & \multicolumn{1}{c}{$\chi$$_{\rm N_2H^+}$} & \multicolumn{1}{c}{$\chi$$_{\rm N_2D^+}$} & \multicolumn{1}{c}{}\\ \noalign{\smallskip} \hline Serpens--FIRS 1 & Model 3 & 1100 & 4.37 & 3.89 & 4.52 & only 10\% of CO~evaporated \\ & {\bf Model 4} & {\bf 1100} & {\bf 2.55} & {\bf 3.77} & {\bf 4.46} & \boldmath{\bf only 10\% survives for $T>100$~K} \\ \noalign{\smallskip} % Cep E-mm & Model 1 & 1100 & 1.48 & 4.12 & 0.71 & \\ % 9.6 & Model 2 & 5000 & 1.51 & 0.86 & 0.45 & \\ % 10.7 & {\bf Model 3} & {\bf 1100} & {\bf 0.91} & {\bf 2.26} & {\bf 1.19} & {\bf only 10\% of CO~evaporated} \\ & Model 4 & 1100 & 1.42 & 2.19 & 1.12 & only 10\% survives for $T>100$~K \\ \noalign{\smallskip} IC~1396~N & Model 3 & 1100 & 2.95 & 4.45 & $>$4.3 & only 10\% of CO~evaporated \\ & {\bf Model 4} & {\bf 1100} & {\bf 1.79} & {\bf 4.35} & {\bf $>$4.0} & \boldmath{\bf only 10\% survives for $T>100$~K} \\ \noalign{\smallskip} % CB3 & {\bf Model 3} & {\bf 1100} & {\bf 1.63} & {\bf 0.76} & {\bf 0.31} & {\bf only 10\% of CO~evaporated} \\ & Model 4 & 1100 & 1.24 & 0.86 & 0.51 & only 10\% survives for $T>100$~K \\ \noalign{\smallskip} NGC~7129$-$FIRS~2 & {\bf Model 3} & {\bf 1100} & {\bf 0.97} & {\bf 1.29} & {\bf 2.05} & {\bf only 10\% of CO~evaporated} \\ & Model 4 & 1100 & 1.39 & 1.48 & 1.73 & only 10\% survives for $T>100$~K \\ \hline \end{tabular} \tablefoot{\tablefoottext{a}{$\chi$ is defined as $\chi = \sqrt[]{[\Sigma (I_{\rm model}-I_{\rm obs})^2]/N} $. Note that this is an absolute error and the comparison among values in different sources is not\\ straightforward. See Figs.~\ref{fig11} to~\ref{fig18}.}} \end{table}