$\begin{figure} \par\includegraphics[width=15cm]{0046fig1.eps} \end{figure}$ Figure 1: Deep optical B + V band image of radio galaxy B2 0648+27. Left: high-contrast plot of B2 0648+27, highlighting the low surface-brightness stellar tail or partial ring. Right: low-contrast plot (logarithmic intensity scale) of the inner region of B2 0648+27.
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In the text

$\begin{figure} \par\includegraphics[width=13cm]{0046fig2.eps} \end{figure}$ Figure 2: Contours of the total intensity H I map from Paper I overlaid onto the deep optical B+V image of B2 0648+27 (grey-scale). Contour levels: 0.22, 0.36, 0.52, 0.71, 0.95, 1.2, 1.5, 1.8, 2.1 $\times 10^{20}$ cm^-2.
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In the text

$\begin{figure} \par\includegraphics[width=15cm]{0046fig1.eps} \end{figure}$	Figure 1: Deep optical B + V band image of radio galaxy B2 0648+27. Left: high-contrast plot of B2 0648+27, highlighting the low surface-brightness stellar tail or partial ring. Right: low-contrast plot (logarithmic intensity scale) of the inner region of B2 0648+27.
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$\begin{figure} \par\includegraphics[width=13cm]{0046fig2.eps} \end{figure}$	Figure 2: Contours of the total intensity H I map from Paper I overlaid onto the deep optical B+V image of B2 0648+27 (grey-scale). Contour levels: 0.22, 0.36, 0.52, 0.71, 0.95, 1.2, 1.5, 1.8, 2.1 $\times 10^{20}$ cm^-2.
Open with DEXTER