\begin{table}%t9
\caption{\label{table9}Observed and derived properties for NGC 92 regions.}
\small%\centerline
 {
\begin{tabular}{ccccccccccccccccccc}
\hline \hline
&&&&&&&& \\[-8pt]
ID & RA& Dec & FUV & NUV & FUV--NUV$^a$ & Age$^b$ & {\it SFR}$_{\rm FUV}$$^c$ &Velocity\\
~ &(2000)&(2000) & ~& ~ & ~ &(Myr)& ($M_{\odot}$ yr$^{-1}$) & (km s$^{-1}$)$^d$\\
\hline
1 &  5.39251  & --48.63508   & 20.04 $\pm$ 0.03 & 19.67 $\pm$ 0.02 & 0.34 $\pm$ 0.07 &       & 0.008 &  3283  \\
2 &  5.39949  & --48.64607   & 20.55 $\pm$ 0.04 & 20.31 $\pm$ 0.01 & 0.19 $\pm$ 0.06 &       & 0.003 &  3289   \\
3 &  5.41036  & --48.64908   & 18.96 $\pm$ 0.02 & 18.77 $\pm$ 0.01 & 0.06 $\pm$ 0.04 &  44.6 & 0.011 &  3294 \\
4 &  5.32479  & --48.64329   & 21.38 $\pm$ 0.07 & 19.99 $\pm$ 0.03 & 0.43 $\pm$ 0.08 &       &       &      \\
5 &  5.33817  & --48.67298   & 21.75 $\pm$ 0.10 & 21.07 $\pm$ 0.05 & 0.38 $\pm$ 0.12 &       &       &       \\
\hline
\end{tabular}}
\medskip
$^a$ Using a fixed aperture of 4\arcsec.  \\ 
$^b$~Age from FUV$-$NUV using Thilker et~al. (\cite{thi07}).  \\
$^c$~{\it SFR} ($M_{\odot}$~yr$^{-1}$) from \mbox{Iglesias-P\'aramo} et~al. (\cite{igl06}) using FUV corrected for internal extinction from \mbox{Gil de Paz} et~al. (\cite{gil07}) and Buat et~al. (\cite{bua05}). Note that these values have uncertainties of typically a factor of~2, given that we have no measured IR/UV~ratios for these objects.  \\ 
$^d$~Estimated from the velocity field. 
\end{table}