Table 2: 408 MHz flux density values for point sources seen along with the SNR. These fluxes are predicted from the spectra published by Vollmer et al. (2005), except for *, where the Northern VLA Sky Survey (NVSS, Condon et al. 1998) was used at 1420 MHz, and the Westerbork Northern Sky Survey (WENSS, Rengelink et al. 1997) at 327 MHz.
\begin{displaymath}\begin{tabular}{lrrccr@{$~\pm~$}l}
\hline\hline
SNR & $\ell...
...161.35&$+$2.90&05 04 44&$+$46 01&180&20\\
\hline
\end{tabular}\end{displaymath}


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