All Figures

$\begin{figure} \par\includegraphics[width=7.2cm,clip]{2758fig1.eps} \end{figure}$ Figure 1: Variations of $\eta =E_{\parallel }/E_{0,\parallel }$ and $\zeta =f(r,P,B)/f_0(p,B)$ with radial distance for $\alpha =65^{\circ }$ and Vela pulsar's parameters. Solid and dashed lines represent $\eta$ and $\zeta$ , respectively. Tow vertical dotted-dash lines represent the inner and outer boundaries of the outer gap.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{2758fig2.eps} \end{figure}$ Figure 2: Plot of the X-ray pulsar luminosity vs. the spin-down luminosity for 19 pulsars. The data points are represented by filled symbols (after Cheng et al. 2004), while model values are represented by open symbols. Pulsars with detected $\gamma$ -ray emission are marked by circles and those with no $\gamma$ -rays detected are marked by squares.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=5.6cm,clip]{2758fig3.eps} \end{figure}$ Figure 3: X-ray luminosity of the Vela pulsar versus the inclination angle. Two horizonal dashed lines represent the upper and lower limits of the observed pulsed X-ray luminosity of the Vela pulsar.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=5.6cm,clip]{2758fig4.eps} \end{figure}$ Figure 4: X-ray luminosity of the Geminga pulsar versus the inclination angle. Two horizonal dashed lines represent the upper and lower limits of the observed pulsed X-ray luminosity of the Geminga pulsar.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.2cm,clip]{2758fig1.eps} \end{figure}$	Figure 1: Variations of $\eta =E_{\parallel }/E_{0,\parallel }$ and $\zeta =f(r,P,B)/f_0(p,B)$ with radial distance for $\alpha =65^{\circ }$ and Vela pulsar's parameters. Solid and dashed lines represent $\eta$ and $\zeta$ , respectively. Tow vertical dotted-dash lines represent the inner and outer boundaries of the outer gap.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6cm,clip]{2758fig2.eps} \end{figure}$	Figure 2: Plot of the X-ray pulsar luminosity vs. the spin-down luminosity for 19 pulsars. The data points are represented by filled symbols (after Cheng et al. 2004), while model values are represented by open symbols. Pulsars with detected $\gamma$ -ray emission are marked by circles and those with no $\gamma$ -rays detected are marked by squares.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=5.6cm,clip]{2758fig3.eps} \end{figure}$	Figure 3: X-ray luminosity of the Vela pulsar versus the inclination angle. Two horizonal dashed lines represent the upper and lower limits of the observed pulsed X-ray luminosity of the Vela pulsar.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=5.6cm,clip]{2758fig4.eps} \end{figure}$	Figure 4: X-ray luminosity of the Geminga pulsar versus the inclination angle. Two horizonal dashed lines represent the upper and lower limits of the observed pulsed X-ray luminosity of the Geminga pulsar.
Open with DEXTER