\begin{table}%t3 %\centering \par \caption{\label{tab:densities}Derived column densities for HOCN and HCNO, and abundance ratios.} \par %\centering \par \begin{tabular}{lcccccccc} \hline \hline\noalign{\smallskip} Source & $N$ (HOCN) & HOCN/H$_2$\tablefootmark{a} & $N$ (HCNO) & HCNO/H$_2$\tablefootmark{a} & $n$(H$_2$) & HNCO/HOCN & HNCO/HCNO & HCNO/HOCN \\ & $10^{10}$~cm$^{-2}$ & $\times10^{13}$ & $10^{10}$~cm$^{-2}$ &$\times 10^{13}$ & 10$^5$~cm$^{-3}$ & & & \\ \hline\noalign{\smallskip} B1-b & 14.3(6)/10(1) & 11/7.7 & 21(1)/17(4)\tablefootmark{b} & 16/13 & 20(5) & 62/80 & 42/47 & 1.5/1.7 \\ L1527 & 3.8(5)/2.7(2) & 13/9.0 & 6(1)/4(1)\tablefootmark{b} & 21/15 & 5(1)\tablefootmark{b} & 58/67 & 34/40 & 1.7/1.7 \\ L1527-B &$\leq$1/1.5 & $\leq$3.3/5.0 & 5(1)/4(1)\tablefootmark{b} & 17/13 & 5(1)\tablefootmark{b} &$\geq$90/53 & 18/20 &$\geq$5/2.7 \\ L1544 & 9(1)/8.6(2) & 6.9/6.6 & 6(3)/6(2)\tablefootmark{b} & 4.6/4.8 & 0.7(2)\tablefootmark{b} & 59/48 & 88/65 & 0.7/0.7 \\ L183 & 7(3)/4.0(2) & 88/53 & 6(2)/5(1)\tablefootmark{b} & 75/66 & 5(1) & 51/63 & 60/50 & 0.8/1.2 \\ TMC-1 &$\leq$0.9/1.9 & $\leq$9/19 &$\leq$1.3/1.4\tablefootmark{b} & $\leq$13/14 & 0.3(1)\tablefootmark{b} \\ IRAS 16293-2422 & 125(4)/160(1) & 3.6/ 4.6 &$\leq$115/60 & $\leq$3.3/1.7 & 2.5(5) & 27/21 &$\geq$30/57 &$\leq$0.9/0.4 \\ \par SgrB2M-B & 2600\tablefootmark{c} & $\approx$260 &$\leq$17 & $\leq$1.7& $\approx$1.4\tablefootmark{a} & 181 &$\geq$30000 &$\leq$0.006 \\ SgrB2M h.c. & 70000\tablefootmark{c} & $\approx$260 &$\leq$5818 & $\leq$22 & $\approx$750\tablefootmark{a} & 90 &$\geq$1031 &$\leq$0.083 \\ SgrB2M ext. & 750\tablefootmark{c} & $\approx$75 &$\leq$14 & $\leq$1.4 & $\approx$1.4\tablefootmark{a} & 230 &$\geq$12143 & $\leq$0.019 \\ SgrB2N h.c. & 670000\tablefootmark{c} &$\approx$5200 &$\leq$79139 & $\leq$609 & $\approx$540\tablefootmark{a} & 313 &$\geq$2654 &$\leq$0.118 \\ SgrB2N ext. & 1600\tablefootmark{c} &$\approx$160 &$\leq$45 & $\leq$4.5 & $\approx$1.4\tablefootmark{a} & 181 &$\geq$6444 &$\leq$0.028 \\ SgrB2S & 4200\tablefootmark{c} & $\approx$420 &$\leq$40 & $\leq$4.0 & $\approx$1.4\tablefootmark{a} & 43 &$>$4500 &$<$0.010 \\ \hline \end{tabular} \tablefoot{L1527-B corresponds to the position $(20'',~-20'')$ of this source, and SgrB2M-B to the offset $(20'',~100'')$ with respect to SgrB2M, h.c. refers to a hot core component, and ext. to the extended gas around this hot core. The first entry in the $N$(HOCN), $N$(HCNO) values, and in the abundances ratios corresponds to the column density obtained from the rotational diagrams, while the second one corresponds to the same parameter obtained from the $LVG$ calculations. Column densities in cold cores for HNCO are from \citet{Mar09}, and those for the GC clouds from \citet{Bru09b}. For IRAS 16293-2422 we have assumed $N({\rm HNCO})=3.4\times10^{13}$ \citep{Dis95}. $^a$ Assumed H$_2$ column densities are: B1-b: $1.3\times10^{23}$~cm$^{-2}$ \citep{Hir99}; L1527: $3\times10^{22}$~cm$^{-2}$ \citep{Jor02}; L1544: $1.3\times10^{23}$~cm$^{-2}$ \citep{War99}; L183: $7.6\times10^{21}$~cm$^{-2}$ \citep{Swa89}; TMC-1(CP): $1\times10^{22}$~cm$^{-2}$ \citep{Cer87}; IRAS 16293-2422: $3.5\times10^{24}$~cm$^{-2}$ \citep{Bot04}; SgrB2M-B, SgrB2S, SgrB2M ext., and SgrB2N ext.: $1\times10^{24}$~cm$^{-2}$ \citep{Lis1990}; SgrB2M h.c.: $2.7\times10^{25}$~cm$^{-2}$ \citep{Liu1999}; and SgrB2N h.c.: $1.3\times10^{25}$~cm$^{-2}$ \citep{Belloche2008}. Source sizes for the GC clouds from \cite{Bru09b}, assumed distance to the GC clouds 8 kpc \citep{Reid1993}. \tablefootmark{b} From \citet{Mar09}. \tablefootmark{c} From \citet{Bru09b}.}\vspace*{2mm} \end{table}