\begin{table}%t5
%\centering
\par
\caption{\label{table:conclusions}Main results.}
%
\par
\small
\begin{tabular}{lll}
\hline\hline
& Kes 79 & G352.7$-$0.1 \\
\hline
Radio flux density &at 74~MHz = 76 Jy  & \\
& at 324~MHz = 39Jy & \\
& at 1.5~GHz = 11 Jy & \\
Radio spectral index& $-0.58$&\\
Distance & 7 kpc& 7.5 kpc\\
Age& $<$15~000 yr & 5000 yr\\
X-ray-to-Radio Luminosity& $\sim$100& $\sim$20\\
Elemental abundances& Shocked CSM and ISM& Ejecta\\
Scenario& Core collapse of an O9 star& Interaction with an asymmetric progenitor wind \\
&within a wind-driven bubble& resulting in a ``barrel-shaped'' SNR\\
& plus projection& plus viewing angle and projection\\
\hline
\end{tabular}\vspace*{-2mm}
\end{table}