\begin{table}%t3
\caption{\label{tab:cr_ellipses}The total flux densities were integrated within ellipses chosen to include the extended emission in the disk and halo. The major axis~$a$, and the minor axis~$b$ for each wavelength~$\lambda$ is presented.}
%\centering
\small
\begin{tabular}{lllll}
\hline\hline 
$\lambda~{\rm [cm]}$ \T\B & $a~{\rm [arcsec]}$ & $a~{\rm [kpc]}$ & $b~{\rm [arcsec]}$ & $b~{\rm [kpc]}$\\
\hline
90 \T & 620 & 12.1 & 392 & 7.6\\ 
20 & 620 & 12.1 & 392 & 7.6\\ 
6.2 & 680 & 13.3 & 430 & 8.4\\ 
3.6 \B & 648 & 12.6 & 400 & 7.8\\
\hline
\end{tabular}
\end{table}