\begin{table}%T3
  \caption{\label{table:radio:vla}Results corresponding to the VLA data. Given are the source
  name, the frequency of the observation, the rms noise of the image,
  the integrated flux density and the source size.}
    %\centerline
{
    \normalsize
    \begin{tabular}[h]{lcccc}
      \hline \hline 
    \multicolumn{1}{c}{Source} &
    \multicolumn{1}{c}{$\nu$} &
    \multicolumn{1}{c}{$\sigma$} &
    \multicolumn{1}{c}{Integ. $S_\nu$} &
    \multicolumn{1}{c}{Size} \\
    \multicolumn{1}{c}{} &
    \multicolumn{1}{c}{(GHz)} &
    \multicolumn{1}{c}{(mJy/beam)} &
    \multicolumn{1}{c}{(Jy)} &
    \multicolumn{1}{c}{($\arcsec$)} 
\\[5pt] \hline \\[-5pt]
IRAS 01045$+$6505& 8.4 &0.29 & 242             & 4.7 \\
IRAS 18032$-$2032& 8.4 &1.24 & 461, 71, 66$^\ddagger$ &$19\times10,4,1^\natural$\\
IRAS 18479$-$0005& 8.4 &1.30 & 2588$^\star$    &$4.8,1.5^\rhd$\\
IRAS 19442$+$2427& 8.4 &0.19 & 80$^\dagger$    &$1,12\times7^\Diamond$\\
IRAS 19598$+$3324& 8.4 &2.57 & 3380            &6\\
DR21        & 8.4 &2.75 & 561, 864$^\lhd$  &$4.4\times3, 6\times3.2^\triangle$\\
IRAS 23133$+$6050& 8.4 &0.74 & 737             & 9 \\[3pt] 
\hline 
      \end{tabular}}
 {\smallskip
 $^\dagger$  Respective flux densities of components~B, C and~D.
 $^\natural$  Respective sizes of components~B, C and~D.
 $^\star$  The two main conponents~A and~B have flux densities of
approximately~1315 and~571~mJy, respectively.
 $^\rhd$  Respective sizes of components~A and~B.
 $^\dagger$  The compact core has a flux density of~32~mJy.
 $^\Diamond$  Sizes of the compact and diffuse components, respectively.
 $^\lhd$  Flux densities of components~A and~B, respectively.
 $^\triangle$  Sizes of components~A and~B, respectively.
}
\end{table}