$\begin{figure} \par\includegraphics[width=7.85cm,clip]{5941fig1.eps}\end{figure}$ Figure 1: Part of the Chandra HRC-I image of the Puppis-A supernova remnant. Besides RX J0822-4300, there are two serendipitous point sources detected in the field of view. They are denoted as source A and B. The optical expansion center of Puppis-A as obtained by Winkler et al. (1988) is marked by a cross.
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In the text

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{5941fig2.eps} \end{figure}$ Figure 2: The best-fitted X-ray positions of RX J0822-4300 in two epochs are marked by crosses. The circles indicate the $1-\sigma$ error. The arrow shows the direction of proper motion inferred from both positions.
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In the text

$\begin{figure} \par\includegraphics[width=7.85cm,clip]{5941fig1.eps}\end{figure}$	Figure 1: Part of the Chandra HRC-I image of the Puppis-A supernova remnant. Besides RX J0822-4300, there are two serendipitous point sources detected in the field of view. They are denoted as source A and B. The optical expansion center of Puppis-A as obtained by Winkler et al. (1988) is marked by a cross.
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$\begin{figure} \par\includegraphics[width=7.9cm,clip]{5941fig2.eps} \end{figure}$	Figure 2: The best-fitted X-ray positions of RX J0822-4300 in two epochs are marked by crosses. The circles indicate the $1-\sigma$ error. The arrow shows the direction of proper motion inferred from both positions.
Open with DEXTER