All Figures

$\begin{figure} \par\includegraphics[width=18cm]{fig1.eps}\end{figure}$ Figure 1: a) Comparison of the model results with the multi-wavelength observations for the SNR G347.3-0.5. The emission from primary particles (electrons and protons), and secondary ${\rm e}^{\pm }$ pairs are indicated by solid line and dashed line, respectively. b) The photon (solid line) and $\nu_\mu+\bar{\nu}_\mu$ (dotted line) spectra of the SNR produced from p-p interactions. The radio data (Lazendic et al. 2004), X-ray data (Slane et al. 1999), EGRET upper limit and VHE $\gamma$ -ray data (Aharonian et al. 2006a) for the whole SNR are indicated. The parameters used are shown in Table 1.
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In the text

$\begin{figure} \par\includegraphics[width=18cm,clip]{fig2.eps}\end{figure}$ Figure 2: a) Comparison of the model results with the multi-wavelength observations for the SNR G266.2-1.2. b) The photon (solid line) and $\nu_\mu+\bar{\nu}_\mu$ (dotted line) spectra of the SNR produced from p-p interactions. The radio data (Duncan and Green 2000), X-ray data (Lemoine-Goumard et al. 2007), and VHE $\gamma$ -ray data (Aharonian et al. 2007), for the whole SNR are indicated. Others are the same as Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=18cm,clip]{fig3.eps}\end{figure}$ Figure 3: a) Comparison of the model results with the multi-wavelength observations for the SNR G8.7-0.1. b) The photon (solid line) and $\nu_\mu+\bar{\nu}_\mu$ (dotted line) spectra of the SNR produced from p-p interactions. The radio data (Odegard et al. 1986; Kassim & Weiler 1990; Green 2006), X-ray data (Cui & Konopelko 2006), and VHE $\gamma$ -ray data (Aharonian et al. 2006b; Enomoto et al. 2006) for the whole SNR are indicated. Others are the same as Fig. 1.
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In the text

$\begin{figure*} \par\includegraphics[width=18cm,clip]{fig4.eps} \end{figure*}$ Figure 4: a) Comparison of the model results with the multi-wavelength observations for the SNR G23.3-0.3. b) The photon (solid line) and $\nu_\mu+\bar{\nu}_\mu$ (dotted line) spectra of the SNR produced from p-p interactions. The radio data (Tian et al. 2007) and VHE $\gamma$ -ray data (Aharonian et al. 2006b; Albert et al. 2006) for the whole SNR are indicated. Others are the same as Fig. 1.
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In the text