All Figures

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{408-m.eps}\hspace*{4mm} \i... ...eps}\hspace*{4mm} \includegraphics[width=7.8cm,clip]{bonn-ns-11.eps}\end{figure}$ Figure 1: In each image OA184 is in the lower half and VRO42.05.01 is in the upper half. The first row of images shows the CGPS maps at 408 MHz ( left) and 1420 MHz ( right). The second row shows the 1420 MHz map convolved to the same resolution as the 408 MHz map ( left) and the 2695 MHz Effelsberg map ( right). The two boxes used for whole SNR T-T plots are shown in the upper right image. The 8 boxes, labeled with letters and used for SNR sub-areas T-T plots, are shown in the upper and lower left images. The direction of North (N) and South (S) is marked on the lower right image.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{oa184-1420.eps}\hspace*{5mm} \includegraphics[width=8cm,clip]{vor_1420.eps}\end{figure}$ Figure 2: Expanded 1420 MHz images of OA184 ( the left) and VRO42.05.01 ( the right) with larger greyscale range.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=5.2cm,clip]{tt-1-oa184.eps}\... ...e*{4mm} \includegraphics[angle=-90,width=5.2cm,clip]{tt-3-vro42.eps}\end{figure}$ Figure 3: Whole SNR 408-1420 MHz T-T plots for OA184 ( first row) and VRO42.05.01 ( second row). From left to right for OA184: plot for map including compact sources ( $\alpha =0.28 \pm 0.10$ ); plot for map with Gaussian fits to compact sources subtracted ( $\alpha =0.21\pm 0.12$ ); plot for compact sources removed from analysis ( $\alpha = 0.23\pm 0.06$ ). The respective values of $\alpha$ for VRO42.05.01 are 0.38 $\pm$ 0.03, 0.36 $\pm$ 0.03 and 0.36 $\pm$ 0.03.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{oa184_spec4.eps}\hspace*{4mm} \includegraphics[width=8.2cm,clip]{vro_spec2.eps}\end{figure}$ Figure 4: Radio spectrum of OA184 ( left) and VRO42.05.01 ( right). OA184 has a best-fit spectral index of 0.32, $\chi ^2 =2.3$ for data corrected for the ridge emission $\alpha _{\rm ridge}=0.8$ and compact sources. VRO42.05.01 has best fit spectral index of 0.32, $\chi ^2 =2.3$ for data corrected for compact sources.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{oa184-1420.eps}\hspace*{5mm} \includegraphics[width=8cm,clip]{vor_1420.eps}\end{figure}$	Figure 2: Expanded 1420 MHz images of OA184 ( the left) and VRO42.05.01 ( the right) with larger greyscale range.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{oa184_spec4.eps}\hspace*{4mm} \includegraphics[width=8.2cm,clip]{vro_spec2.eps}\end{figure}$	Figure 4: Radio spectrum of OA184 ( left) and VRO42.05.01 ( right). OA184 has a best-fit spectral index of 0.32, $\chi ^2 =2.3$ for data corrected for the ridge emission $\alpha _{\rm ridge}=0.8$ and compact sources. VRO42.05.01 has best fit spectral index of 0.32, $\chi ^2 =2.3$ for data corrected for compact sources.
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