\begin{table}%t2
\caption{\label{tab2}Properties of clusters younger than $\log (t_{\rm c})$~= 8.00 in the LMC.}
\small%\centerline
 {
\begin{tabular}{l|*{8}{c}}
\hline\hline %\noalign{\smallskip}
&&&&&&&&\\[-3mm]
Identifier & $\log (\rm age)$    &  $\Delta$ age &  Radius   &  $\Delta$ radius & $M_{\rm total}$ & $\Delta M_{\rm total}$ & $\log (\rho)$ & $\Delta \rho$\\
           & [Myr]        &               &  [pc]     &                  & [\Msun]     & &           [\Msun/pc$^{-3}$] &          \\
           \hline  %\noalign{\smallskip}
	  &&&&&&&&\\[-3mm] 
NGC 1805$^1$ &   7.0   &  0.3  &  1.33  &  0.06 & 3.52 & 0.13 & 2.54 & 0.2\\
NGC 1818$^1$ &   7.4   &  0.3  &  2.45  &  0.09 & 4.13 & 0.15 & 2.35 & 0.2\\
NGC 1984$^1$ &   7.06  &  0.3  &  0.99  &  0.07 & 3.38 & 0.24 & 2.79 & 0.2\\
NGC 2004 $^1$&   7.30  &  0.2  &  1.57  &  0.13 & 4.43 & 0.38 & 2.32 & 0.2\\
NGC 2011$^1$ &   6.99  &  0.3  &  1.17  &  0.12 & 3.47 & 0.14 & 3.24 & 0.12\\
NGC 2100$^2$ &   7.20  &  0.3  &  1.14  &  0.14 & 4.43 & 0.13 & 3.05 & 0.2\\
R 136$^1$    &   6.48  &  0.18 &  0.32  &  0.02 & 4.55 & 0.21 & 4.47 & 0.08\\
\hline
\end{tabular}}
\medskip
$^1$ Mackey \& Gilmore (\cite{mackey:03a}); and $^2$ McLaughlin \& \mbox{van der Marel} (2006).
\end{table}