All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=7.7cm,clip]{1686f1a.ps}\vspace*{5mm} \includegraphics[angle=-90,width=7.7cm,clip]{1686f1b.ps}\end{figure}$ Figure 1: Colour-colour diagrams for the two WFC fields around NGC 205. Colours are computed from instrumental magnitudes, so that the zero points of the x and y axes are arbitrary.
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In the text

$\begin{figure} \par\includegraphics[width=11cm,clip]{1686fig2.ps}\end{figure}$ Figure 2: Digitized Sky Survey image of an area of 34 $^\prime$ $\times$ 34 $^\prime$ around NGC 147. North is at the top, East to the left. Candidate PNe are marked with crosses.
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In the text

$\begin{figure} \par\includegraphics[width=11cm,clip]{1686fig3.ps}\end{figure}$ Figure 3: Digitized Sky Survey image of an area of 34 $^\prime$ $\times$ 34 $^\prime$ around NGC 185. North is at the top, East to the left. Candidate PNe are marked with crosses.
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In the text

$\begin{figure} \par\includegraphics[width=11cm,clip]{1686fig4.eps}\end{figure}$ Figure 4: Digitized Sky Survey image of an area of 50 $^\prime$ $\times$ 50 $^\prime$ around NGC 205 (a portion of the disk of M 31 is visible in the bottom-left corner of the field). North is at the top, East to the left. Candidate PNe are marked with crosses. The ellipse at 1.5 tidal radii is indicated.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{1686fig5.eps}\end{figure}$ Figure 5: The PN surface density at increasing distances from M 31 in strips parallel to its major axis, and outside 1.5 tidal radii from the centre of NGC 205 (see text). The zero point of the x-axis corresponds to the inner limit of our observed field. The dashed lines indicate the range of distances within which NGC 205 is located.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{1686fig6.eps}\end{figure}$ Figure 6: The luminosity function of the 35 candidate PNe within 1.5 tidal radii from the centre of NGC 205. The fit down to the completeness limit of our images is indicated by the solid line.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{1686fig7.eps}\end{figure}$ Figure 7: Histogram of the absolute magnitudes of the candidate PNe in NGC 147 (dashed histogram) and NGC 185 (thick solid line). The completeness limits of our survey are indicated for each galaxy by the arrows in the upper part of the diagram.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.7cm,clip]{1686f1a.ps}\vspace*{5mm} \includegraphics[angle=-90,width=7.7cm,clip]{1686f1b.ps}\end{figure}$	Figure 1: Colour-colour diagrams for the two WFC fields around NGC 205. Colours are computed from instrumental magnitudes, so that the zero points of the x and y axes are arbitrary.
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$\begin{figure} \par\includegraphics[width=11cm,clip]{1686fig2.ps}\end{figure}$	Figure 2: Digitized Sky Survey image of an area of 34 $^\prime$ $\times$ 34 $^\prime$ around NGC 147. North is at the top, East to the left. Candidate PNe are marked with crosses.
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$\begin{figure} \par\includegraphics[width=11cm,clip]{1686fig3.ps}\end{figure}$	Figure 3: Digitized Sky Survey image of an area of 34 $^\prime$ $\times$ 34 $^\prime$ around NGC 185. North is at the top, East to the left. Candidate PNe are marked with crosses.
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$\begin{figure} \par\includegraphics[width=11cm,clip]{1686fig4.eps}\end{figure}$	Figure 4: Digitized Sky Survey image of an area of 50 $^\prime$ $\times$ 50 $^\prime$ around NGC 205 (a portion of the disk of M 31 is visible in the bottom-left corner of the field). North is at the top, East to the left. Candidate PNe are marked with crosses. The ellipse at 1.5 tidal radii is indicated.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{1686fig5.eps}\end{figure}$	Figure 5: The PN surface density at increasing distances from M 31 in strips parallel to its major axis, and outside 1.5 tidal radii from the centre of NGC 205 (see text). The zero point of the x-axis corresponds to the inner limit of our observed field. The dashed lines indicate the range of distances within which NGC 205 is located.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{1686fig6.eps}\end{figure}$	Figure 6: The luminosity function of the 35 candidate PNe within 1.5 tidal radii from the centre of NGC 205. The fit down to the completeness limit of our images is indicated by the solid line.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{1686fig7.eps}\end{figure}$	Figure 7: Histogram of the absolute magnitudes of the candidate PNe in NGC 147 (dashed histogram) and NGC 185 (thick solid line). The completeness limits of our survey are indicated for each galaxy by the arrows in the upper part of the diagram.
Open with DEXTER