\begin{table}%t5 \caption{\label{t5}Results of fits to the spectra observed at Medicina.} \par %\centerline { \begin{tabular}{ccccccc} \hline\hline\noalign{\smallskip} Name & Line & $T_{\rm MB}$ & rms & $V_{\rm LSR}$ & $\Delta V$ & $\tau_{\rm tot}$ \\ & & (K) & (mK) & (km s$^{-1}$) & (km s$^{-1}$) & \\ \hline G12.22--0.12\tablefootmark{a} & (1,1) & 0.52(0.07) & 81 & +27.0(0.2) & 4.5(0.4) & 0.6 \\ & (2, 2) & 0.26(0.06) & 72 & +25.6(0.4) & 6.7(1.6) & --\tablefootmark{b} \\ G12.22--0.12M & (1, 1) & 0.70(0.08) & 127 & +28.2(0.1) & 3.1(0.4) & 0.1 \\ & (2, 2) & 0.36(0.08) & 118 & +28.7(0.3) & 2.8(0.6) & --\tablefootmark{b} \\ G23.44--0.18 & (1, 1) & 1.02(0.13) & 153 & +99.4(0.2) & 4.7(0.3) & 4.6 \\ & (2, 2) & 0.53(0.08) & 112 & +100.4(0.2) & 4.0(0.7) & 1.2 \\ G31.28+0.06 & (1, 1) & 0.29(0.03) & 27 & +108.6(0.1) & 4.0(0.2) & 2.7 \\ & (2, 2) & 0.12(0.01) & 22 & +108.5(0.2) & 4.6(0.7) & 0.6 \\ G32.74--0.07 & (1, 1) & 0.31(0.03) & 41 & +37.5(0.1) & 3.4(0.2) & 2.2 \\ & (2, 2) & 0.18(0.03) & 35 & +37.3(0.2) & 3.9(0.9) & --\tablefootmark{b} \\ G35.03+0.35 & (1, 1) & 0.26(0.02) & 38 & +52.9(0.1) & 3.2(0.3) & 1.1 \\ & (2, 2) & 0.15(0.02) & 31 & +53.3(0.2) & 2.8(0.6) & --\tablefootmark{b} \\ G35.20--0.74\tablefootmark{a} & (1, 1) & 1.19(0.04) & 30 & +33.7(0.1) & 3.1(0.1) & 2.3 \\ & (2, 2) & 0.66(0.02) & 26 & +33.7(0.1) & 3.8(0.2) & --\tablefootmark{b} \\ G35.20--1.74 & (1, 1) & 0.44(0.03) & 26 & +42.6(0.1) & 2.9(0.2) & 1.7 \\ & (2, 2) & 0.27(0.02) & 26 & +42.7(0.1) & 2.9(0.3) & 1.1 \\ G43.89--0.38 & (1, 1) & 0.56(0.07) & 105 & +54.3(0.1) & 3.0(0.3) & 1.7 \\ & (2, 2) & 0.19(0.04) & 67 & +55.0(0.4) & 5.3(1.0) & --\tablefootmark{b} \\ G48.61+0.02 & (1, 1) & 0.08(0.01) & 19 & +19.5(0.2) & 3.7(0.5) & 1.0 \\ & (2, 2) & 0.03(0.01) & 19 & +19.4(0.5) & 3.1(1.1) & --\tablefootmark{b} \\ G75.78+0.34 & (1, 1) & 0.69(0.06) & 87 & --0.5(0.1) & 4.1(0.3) & 0.6 \\ & (2, 2) & 0.38(0.05) & 81 & --0.1(0.2) & 3.5(0.7) & --\tablefootmark{b} \\ \hline \end{tabular}} \par \tablefoot{\tablefoottext{a}{Given the spatial resolution of the Medicina antenna, the spectra collect the contributions due to both A and B cores (see Figs. 7--10).} \tablefoottext{b}{Satellites not detected.}}\vspace*{-2mm} \end{table}