\begin{table}%t1
\caption{Emission line fluxes.} \label{emlines}
\small
%\centerline
{
\begin{tabular}{llllll}
\hline \hline \noalign{\smallskip}
Line ratios & Region 1 &  Region 2 & Region 3 & Region 4 & Region 5 \\
 & 29\farcs3 & 54\farcs4 & 18\farcs4 & 85\farcs6 & 83\farcs7 \\
\noalign{\smallskip}
 \hline
\noalign{\smallskip}
$[$N II$]$ $\lambda$ 6583/ H$\alpha$            & 0.76 $\pm$ 0.05 & 0.70 $\pm$ 0.08 & 0.60 $\pm$ 0.10 & 0.21 $\pm$ 0.11  & 0.15 $\pm$ 0.06\\
$[$S II$]$ $\lambda$ 6716 + 6731/ H$\alpha$     & 0.99 $\pm$ 0.09 & 0.88 $\pm$ 0.14 & 0.80 $\pm$ 0.18 & 0.15 $\pm$ 0.13  & 0.21 $\pm$ 0.07\\
$[$S II$]$ $\lambda$6716/$[$S II$]$ $\lambda$6731 & 1.46 $\pm$ 0.18 & 1.52 $\pm$ 0.33 & 1.34 $\pm$ 0.44 & $\ga$1.3 & $\ga$1.5 \\
 \hline
\end{tabular}}
\medskip
$^a$ Lower limits to the $[$S II$]$
$\lambda$6716/$[$S II$]$ $\lambda$6731 ratio are provided assuming
a 1$\sigma$ upper limit to the flux of the $\lambda$6731 line, if
the line is not detected.
\end{table}