\begin{table}%t9 \caption{\label{t9}Ammonia column densities derived from the VLA maps.} %\centerline { \begin{tabular}{cccc} \hline\hline\noalign{\smallskip} Name & $T_{\rm rot}$\tablefootmark{a} & $N_{\rm 22}$\tablefootmark{a} & $N_{\rm tot}$\tablefootmark{a} \\ & (K) & (cm$^{-2}$) & (cm$^{-2}$) \\ \hline \multicolumn{4}{c}{Extended ammonia emission$^b$} \\ G23.44--0.18 & $\ge$9 & 3--30 $\times$ 10$^{14}$ & 1--8 $\times$ 10$^{16}$ \\ G31.24--0.11 & $\ge$14 & 0.6--45 $\times$ 10$^{14}$ & 0.2--2 $\times$ 10$^{16}$\tablefootmark{b} \\ G32.74--0.07 & $\ge$9 & 0.4--45 $\times$ 10$^{14}$ & 0.2--12 $\times$ 10$^{16}$\tablefootmark{b} \\ G35.03+0.35 & $\ge$6 & 2--30 $\times$ 10$^{14}$ & 0.1--18 $\times$ 10$^{17}$ \\ G43.89--0.38 & $\ge$6 & 0.2--41 $\times$ 10$^{14}$ & 0.2--230 $\times$ 10$^{16}$\tablefootmark{b} \\ \hline \multicolumn{4}{c}{Ammonia cores} \\ G12.22--0.12A & $\ge$47 & 4--9 $\times$ 10$^{16}$ & 2--4 $\times$ 10$^{17}$ \\ G12.22--0.12B & $\ge$36 & 2--4 $\times$ 10$^{16}$ & 7--17 $\times$ 10$^{16}$ \\ G12.22--0.12M & $\ge$29 & 1--5 $\times$ 10$^{16}$ & 8--12 $\times$ 10$^{16}$ \\ G31.28+0.06 & $\ge$25 & 6--26 $\times$ 10$^{15}$ & 4--10 $\times$ 10$^{16}$ \\ G35.20--0.74A & $\ge$49 & 2--3 $\times$ 10$^{16}$ & 6--12 $\times$ 10$^{16}$ \\ G35.20--0.74B & $\ge$31 & 2--7 $\times$ 10$^{15}$ & 1--3 $\times$ 10$^{16}$ \\ G48.61+0.02 & $\ge$7 & 1--14 $\times$ 10$^{15}$ & 5--210 $\times$ 10$^{16}$ \\ G75.78+0.34 & $\ge$28 & 3--9 $\times$ 10$^{15}$ & 2--4 $\times$ 10$^{16}$ \\ \hline \end{tabular}} \par \tablefoot{\tablefoottext{a}{Given the low spectral resolution (see Sect. 2.2) of the NH$_3$(3,~3) spectra, we estimated a lower limit for $T_{\rm rot}$ as the maximum $T_{\rm MB}$ value shown by the (2, 2) and (3, 3) spectra. As an upper limit we arbitrarily assumed 100 K.} \tablefoottext{b}{The column densities derived for G31.24--0.11, G32.74--0.07, and G43.89--0.38 are very approximative due to no optical depth measurement (see Table 5): in this case $\tau_{\rm tot}$ = 0.1--1 has been arbitrarily assumed.}} \end{table}