\begin{table}%t4 \caption{\label{t:hco}\HCOp\ observations. Isotopes are abbreviated as 12~(\HCOp), 13~(H$^{13}$CO$^+$), and 18~(HC$^{18}$O$^+$).} \par %\centering \small \begin{tabular}{lc@{~}crcccc @{}c@{}c@{}c l} \hline\hline\noalign{\smallskip} & & &\TL, K $^a$ &\multicolumn{2}{c}{${v_{\rm LSR},\mkm}\ ^b$} & {10\% width $^c$}\ & Profile & \multicolumn{2}{c}{${\rm Size, arcsec}$}& PA & \\ source& isotope & line & peak ¢roid& abs.&\km & type & $\Delta l$ & $\Delta b$ & deg. &remark \\ \hline SGRB2MC & 12 &3--2 & 9.7 & ? & 70.6& 67.7 & &&& &complex profile,\\ & 13 &3--2 & 4.0 & 56.7 & 62.5& 30.7 & R & &&& broad abs. below cont. \\ G10.62-0.38 & 12 &3--2 & 21.5 & --5.1 & 0.0 & 18.1 & &22.8 & 20.5 & 84 &self-abs., \SOtwo \\ & 13 &3--2 & 4.2 & --2.94& --2.1 & 12.0 & B & \\ & 18 &3--2 & 1.0 & --2.46& --- & & & \\ G10.96+0.01E& 12 &3--2 & ${<}0.045$ & & & & & & & & (1)\\ G10.96+0.01W& 12 &3--2 &${\sim}0.2$&30.0& ---& ${\sim}10$& &&& &marginal \\ G12.21-0.10 & 12 &3--2 & 5.8 & 24.1 & --- & 13.5 & & 16.2 & 12.8 & 71 &\SOtwo\\ G25.5+0.2A & 12 &3--2 & ${<}0.20$ & & & & & & & & (1)\\ G28.20-0.04N& 12 &3--2 & 3.6 & ? & 45.0& 22.9 & & 16.6 & 14.2 & 73 &\HCOpd\ self-abs.; \SOtwo \\ & 13 &3--2 & 0.61 & 43.0 & 44.3& 11.9 & B & \\ & 18 &3--2 & 0.13 & 44.0 & --- & & & \\ G28.20-0.04S& 12 &1--0 & 0.22 & 41.5 & --- & ${\sim}8$& C &&& & \\ G28.28-0.36 & 12 &3--2 & 1.9 & 47.1 & --- & ${\sim}12$ &\\ G29.96-0.02 & 12 &3--2 & 9.6 & 97.7 & --- & 10.9 & & 19.2 & 17.6 & 62 &wings ?\\ G30.54+0.02 & 12 &3--2 & 2.8 & 48.3 & --- & 8.1 & & 21 & 18 & $--12$ &red em. wing \\ G31.41+0.31 & 12 &3--2 & 3.1 & ? & 98.5& ${\sim}23$ & & 18 & 14 & 65 &\HCOp\ self-abs. below cont;\SOtwo\\ & 13 &3--2 & 1.4 & 98.0 & 98.8& 9.6 & B &&& & line-rich \\ G32.80+0.19 & 12 &3--2 & 4.2 & ? & 14.5& 17.3 & & 20 & 19 & $-11$ &broad self-abs. \\ & 13 &3--2 & 1.3 & 14.9 & 14.1& 12.9 & B & \\ G33.13-0.09 & 12 &3--2 & 1.6 & 76.6 & 76.4& 12.7 & & 25 & 17 & $-85$ \\ & 13 &3--2 & 0.32 & 76.6 & 76.1& 7.5 & R & \\ G33.560+0.20& 12 &3--2 & ${<}0.09$ & & & & & & & & (1) \\ G34.26+0.15B& 12 &3--2 & 13.2 & ? & 60.8& 14.3 & & 29 & 25 & $-27$ & \SOtwo, OCS, line-rich\\ & 13 &3--2 & 2.8 & 58.7 & 60.1& 8.7 & B & \\ G35.20-1.74 & 12 &3--2 & 6.5 & ? & 43.7& 11.3 & & 27 & 26 & 61 \\ & 13 &3--2 & 0.94 & 44.5 & 43.5& 7.9 & R & \\ & 18 &3--2 & 0.11 & 45.5 & --- & & & \\ G41.71+0.11 & 12 &3--2 & $<0.11$ & & & & & & & & (1)\\ G43.89-0.78 & 12 &3--2 & 1.8 & ? & 55.2& ${\sim}15$ & & 21 & 21 & --4 \\ & 13 &3--2 & 0.64 & 54.0 & 55.1& 6.5 & R & \\ G45.07+0.13 & 12 &3--2 & 6.4 & ? & --- & 20.7 & & 15 & 14 & $-79$ &asymm. profile \\ & 13 &3--2 & 1.2 & 58.0 & & 10.8 & & \\ G45.12+0.13 & 12 &3--2 & 6.3 & 59.8 & --- & 11.6 & & 38 & 35 & 28 &red em. wing \\ W51D & 12 &3--2 & 14.9 & ${\sim}60.0$ & 51.1& 20.8 & & 21 & 15 & $-86$ &complex profile, \SOtwo\\ & 13 &3--2 & 1.9 & 60.9 & 11.6&${\sim}52$& R & \\ & 12 &1--0 & 10.5 & ${\sim}60.0$ & 52.6& 16.8 & &&& &complex profile \\ G70.29+1.60 & 12 &3--2 & 8.5 & --23.0& --- & 14.6 & & 24 & 19 & $-87$ &weak wings\\ & 12 &1--0 & 7.9 & --23.9& --- & 15.2 & &&& &weak wings \\ G81.67+0.53 & 12 &3--2 & 12.3 & ? & --1.8& 27.2 & & 33 & 27 & 4 &weak wings \\ & 13 &3--2 & 2.1 & --3.3 & --1.9& 11.9 & B & \\ G81.68+0.54 & 12 &3--2 & 4.1 & --2.7 & --2.4& 25.9 & &&& &weak wings \\ & 13 &3--2 & 1.8 & --2.5 & --2.2& 4.6 & B & \\ G111.612 & 12 &1--0 & 6.0 &--56.6 & --- & 5.9 & &\\ NGC 7538IRS1 & 12 &3--2 & 7.5 &--57.5 & --- & 13.7 & & 59 & 48 & 48 & complex profile, red wing \\ NGC 7538IRS2 & 12 &1--0 & 2.9 &--60.0 &--62.7& 17.8 & &&& &complex profile, wings\\ \hline \end{tabular} \tablefoot {The size of the \HCOpd\ source is approximated by an ellipse with major axis~$\Delta l$, its position angle~PA, and minor axis~$\Delta b$. \\ \tablefoottext{a}{Typical rms errors are 150, 50, and 20~mK for the \HCOp, H$^{13}$CO$^+$, and HC$^{18}$O$^+$~isotopes (see also Fig.~\ref{f:isotopes});} \tablefoottext{b}{errors are ${\la}0.8$~\km\ (half the channel spacing);} \tablefoottext{c}{the error is ${\la}1$~\km\ for values preceded by~$\sim$, the other values have errors of ${\sim}0.1$~\km.} \\ (1)~1$\sigma$ upper limit for 2.1~\km\ spectral resolution over a~${\pm}80$~\km\ range; ?~line profile too complex.} \vspace*{6.8mm} \end{table}