\begin{table}%t12
\caption{\label{mass}Physical parameters of IRAS~00213$+$6530.}
\small%\centerline
 {
\begin{tabular}{lcccc}
\hline\hline\noalign{\smallskip}
& Mass$^{a}$ &$\Delta v^{b}$ &$\theta~^{c}$
&$M_{{\rm vir}}^{d}$ \\
Region  &  (\mo)  &(\kms) & (arcsec) &(\mo)\\	
\hline
MM1     &\phb3.5   &0.85  &\phn7&  1.3\\
Southern cloud        &$<$0.3         &0.65  &\phn6&  0.7\\ 
MM2   &\phb1.1  &0.75  &11&  1.6\\
\hline
\end{tabular}}
\medskip
$^a$ Estimated as $M=\mu_{{\rm H_2}}m_{{\rm H}}\sum N({\rm H_{2}})\Delta A$, where $N({\rm H}_{2})$ is taken from the \hh\
column density map, $\Delta A$ is the pixel area, and a mean molecular mass per \hh\ molecule  $\mu_{{\rm H_2}}=2.8$, which corresponds to
a 10\% helium abundance. 
$^b$ Intrinsic line width of the magnetic hyperfine components. 
$^c$ Deconvolved geometrical mean size of the major and minor axes of the source, obtained from a 2D Gaussian fit.
$^d$ Estimated for a density distribution $n\propto$~$r^{-2}$.
\end{table}