\begin{table}%t5 \par \caption{\label{tab5}Abundance profiles derived from the observations.} \small%\centering \par \begin{tabular}{lllllllc} \hline \hline \multicolumn{1}{l}{\bf Serpens-FIRS 1} & \multicolumn{1}{c}{$X_0$} & \multicolumn{1}{c}{$R_0$ (AU)} & \multicolumn{1}{c}{$X_1$} & \multicolumn{1}{c}{$R_1$} (AU) & \multicolumn{1}{c}{$X_2$} & \multicolumn{1}{c}{rms (K km s$^{-1}$)} & \multicolumn{1}{c}{Diameter($''$)/{\it HPBW}($''$)}\\ \hline C$^{18}$O~ & 1.4~$\times$~10$^{-7}$ & \multicolumn{1}{l}{2000} & $<$7~$\times$~10$^{-9}$ & \multicolumn{1}{l}{6000} & 1.1~$\times$~10$^{-7}$ & 0.27 & 2.3 \\ N$_2$H$^+$ & 4.0~$\times$~10$^{-10}$ & \multicolumn{1}{l}{3000} & $<$3~$\times$~10$^{-11}$ & \multicolumn{1}{l}{6000} & 2.5~$\times$~10$^{-10}$ & 0.29 & 1.9\\ \hline N$_2$D$^+$ & \multicolumn{3}{c}{$<$2~$\times$~10$^{-12}$} & \multicolumn{1}{l}{6000} & 1.9~$\times$~10$^{-11}$ & 0.6 & 3.1 \\ \hline $T_{\rm ev}^*$ (K) & \multicolumn{6}{l}{20 } \\ $n_{\rm ev}^*$ (cm$^{-3}$) & \multicolumn{6}{l}{2.4~$\times$~10$^6$} \\ \hline \multicolumn{1}{l}{\bf Cep E-mm} & \multicolumn{1}{c}{$X_0$} & \multicolumn{1}{c}{$R_0$ (AU)} & \multicolumn{1}{c}{$X_1$} & \multicolumn{1}{c}{$R_1$} (AU) & \multicolumn{1}{c}{$X_2$} & \multicolumn{1}{c}{rms (K km s$^{-1}$)} \\ \hline C$^{18}$O~ & 6.0~$\times$~10$^{-8}$ & \multicolumn{1}{l}{3500} & \multicolumn{3}{c}{1.1~$\times$~10$^{-7}$~$\times$~($r$/35~800)} & 0.24 & 4.4 \\ N$_2$H$^+$ & 2.4~$\times$~10$^{-10}$ & \multicolumn{1}{l}{6000} & \multicolumn{3}{c}{2.5~$\times$~10$^{-10}$~$\times$~($r$/35~800)} & 0.28 & 3.7 \\ \hline N$_2$D$^+$ & \multicolumn{5}{c}{7.0~$\times$~10$^{-12}$} & & 6.1\\ \hline $T_{\rm ev}$ (K) & \multicolumn{6}{l}{20 } \\ $n_{\rm ev}$ (cm$^{-3}$) & \multicolumn{6}{l}{1.0~$\times$~10$^6$} \\ \hline \multicolumn{1}{l}{\bf IC 1396 N} & \multicolumn{1}{c}{$X_0$} & \multicolumn{1}{c}{$R_0$ (AU)} & \multicolumn{1}{c}{$X_1$} & \multicolumn{1}{c}{$R_1$} (AU) & \multicolumn{1}{c}{$X_2$} & \multicolumn{1}{c}{rms (K km s$^{-1}$)} \\ \hline C$^{18}$O~ & 6.0~$\times$~10$^{-8}$ & \multicolumn{1}{l}{5500} & \multicolumn{3}{c}{1.25~$\times$~10$^{-7}$~$\times$~($r$/29~600)} & 0.24 & 3.5 \\ N$_2$H$^+$ & 4.2~$\times$~10$^{-10}$ & \multicolumn{1}{l}{10~000} & 1.0~$\times$~10$^{-11}$ & \multicolumn{1}{l}{15~000} & 1.8~$\times$~10$^{-10}$ & 0.50 & 3.0 \\ N$_2$D$^+$ & \multicolumn{5}{c}{$<$7~$\times$~10$^{-12}$} & & 4.9 \\ \hline $T_{\rm ev}$ (K) & \multicolumn{6}{l}{19 } \\ $n_{\rm ev}$ (cm$^{-3}$) & \multicolumn{6}{l}{7.0~$\times$~10$^5$} \\ \hline \multicolumn{1}{l}{\bf CB3} & \multicolumn{1}{c}{$X_0$} & \multicolumn{1}{c}{$R_0$ (AU)} & \multicolumn{1}{c}{$X_1$} & \multicolumn{1}{c}{$R_1$} (AU) & \multicolumn{1}{c}{$X_2$} & \multicolumn{1}{c}{rms (K km s$^{-1}$)} \\ \hline C$^{18}$O~ & 1.3~$\times$~10$^{-7}$ & \multicolumn{1}{l}{25~000} & $<$3.0~$\times$~10$^{-8}$ & \multicolumn{1}{l}{60~000} & 9.0~$\times$~10$^{-7}$ & 0.24 & 3.7 \\ \hline N$_2$H$^+$ & \multicolumn{5}{c}{6.5~$\times$~10$^{-10}$} & 0.45 & 3.1 \\ N$_2$D$^+$ & \multicolumn{5}{c}{3.0~$\times$~10$^{-11}$} & & 5.1 \\ \hline $T_{\rm ev}$ (K) & \multicolumn{6}{l}{15 } \\ $n_{\rm ev}$ (cm$^{-3}$) & \multicolumn{6}{l}{3.0~$\times$~10$^4$} \\ \hline \multicolumn{1}{l}{\bf NGC 7129$-$FIRS 2} & \multicolumn{1}{c}{$X_0$} & \multicolumn{1}{c}{$R_0$ (AU)} & \multicolumn{1}{c}{$X_1$} & \multicolumn{1}{c}{$R_1$} (AU) & \multicolumn{1}{c}{$X_2$} & \multicolumn{1}{c}{rms (K km s$^{-1}$)} \\ \hline C$^{18}$O~ & \multicolumn{5}{c}{4.0~$\times$~10$^{-8}$} & 0.4 & 1.4 \\ N$_2$H$^+$ & \multicolumn{5}{c}{4.7~$\times$~10$^{-10}$} & 0.4 & 1.1 \\ \hline N$_2$D$^+$ & $<$3.0~$\times$~10$^{-12}$ & \multicolumn{1}{l}{9000} & 4.5~$\times$~10$^{-11}$ & \multicolumn{1}{l}{11~000} & $<$3.0~$\times$~10$^{-12}$ & 0.13 & 2.7 \\ \hline \end{tabular} \tablefoot{\tablefoottext{*}{Temperature and density at the CO~evaporation radius.}} \vspace*{2mm} \end{table}