All Figures

$\begin{figure} \par\includegraphics[width=7cm,clip]{1155fig1.eps}\end{figure}$ Figure 1: The evolution of the radial profiles of an undimensional coefficient of emission $\varepsilon _\nu (r)$ (Eq. (22)) in its dependence on the inputparameters.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{1155fig2.eps}\end{figure}$ Figure 2: Normalized projected radial profiles of synchrotron emission for ${\cal M}_{\rm0} = 100$ and different sets of parameters $({\cal M}_{\rm s} ,k ,c_{\rm 1} )$ .
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{1155fig3.eps} % \end{figure}$ Figure 3: The dependence of undimensional luminosity (Eq. (25)) on ${\cal M}_{\rm s}$ . The tracks are labeled with input parameters $({\cal M}_{\rm 0}, ~k, ~c_{\rm 1} )$ .
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{1155fig4.eps} % \end{figure}$ Figure 4: The dependence of undimensional surface brightness (Eq. (28)) on ${\cal M}_{\rm s}$ . Curves are labeled with input parameters $({\cal M}_{\rm 0}, ~k, ~c_{\rm 1} )$ .
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{1155fig5.eps}\end{figure}$ Figure 5: The evolution of the integral radio spectral index with shock Mach number. Curves are marked by the values of parameters ${\cal M}_{\rm0} ,k ,c_{\rm 1}$ .
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{1155fig6.eps} % \end{figure}$ Figure 6: $\Sigma_{\rm 1~~GHz} - D$ diagram for 158 composite and shell-type SNRs and SNR candidates in our Galaxy (filled circles), M 31 (small crosses), M 33 (open diamonds), LMC (open triangles), SMC (filled triangles), NGC 300 (filled diamond), NGC 6946 ( $\times$ 's), NGC 7793 (open circles), and IC 1613 (asterisk). Galactic loopsare shown as large crosses and the only candidate for HNR as a large open circle. Forseveral galactic SNRs, error bars due to the distance uncertainty are shown, and for one galactic SNR (HB 9) only upper limit for the distance is known. Theoretical $\Sigma - D$ tracks are labeled according to the numeration in Table 2.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{1155fig7.eps} % \end{figure}$ Figure 7: 1.4 GHz flux density-diameter relation for 121 SNRs in nearby normal galaxies + Cas A SNR, if they are at $1~\rm {kpc}$ distance. Symbols and lines have the same meanings as in Fig. 6.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{1155fig1.eps}\end{figure}$	Figure 1: The evolution of the radial profiles of an undimensional coefficient of emission $\varepsilon _\nu (r)$ (Eq. (22)) in its dependence on the inputparameters.
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$\begin{figure} \par\includegraphics[width=7.3cm,clip]{1155fig2.eps}\end{figure}$	Figure 2: Normalized projected radial profiles of synchrotron emission for ${\cal M}_{\rm0} = 100$ and different sets of parameters $({\cal M}_{\rm s} ,k ,c_{\rm 1} )$ .
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$\begin{figure} \par\includegraphics[width=7.1cm,clip]{1155fig3.eps} % \end{figure}$	Figure 3: The dependence of undimensional luminosity (Eq. (25)) on ${\cal M}_{\rm s}$ . The tracks are labeled with input parameters $({\cal M}_{\rm 0}, ~k, ~c_{\rm 1} )$ .
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$\begin{figure} \par\includegraphics[width=7.1cm,clip]{1155fig4.eps} % \end{figure}$	Figure 4: The dependence of undimensional surface brightness (Eq. (28)) on ${\cal M}_{\rm s}$ . Curves are labeled with input parameters $({\cal M}_{\rm 0}, ~k, ~c_{\rm 1} )$ .
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$\begin{figure} \par\includegraphics[width=7.1cm,clip]{1155fig5.eps}\end{figure}$	Figure 5: The evolution of the integral radio spectral index with shock Mach number. Curves are marked by the values of parameters ${\cal M}_{\rm0} ,k ,c_{\rm 1}$ .
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{1155fig7.eps} % \end{figure}$	Figure 7: 1.4 GHz flux density-diameter relation for 121 SNRs in nearby normal galaxies + Cas A SNR, if they are at $1~\rm {kpc}$ distance. Symbols and lines have the same meanings as in Fig. 6.
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