All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{1045fig1.eps} \end{figure}$ Figure 1: i-band CCD image of And II obtained at the 2.56 m Nordic Optical Telescope. The field covers $\approx$ 6 $\hbox {$.\mkern -4mu^\prime $ }$ 5 $\times$ 6 $\hbox {$.\mkern -4mu^\prime $ }$ 5, i.e. most of the galaxy with its center somewhat displaced to the upper right. North is up and east to the left.
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{1045fig2.eps} \end{figure}$ Figure 2: Colour-magnitude diagrams for the 2307 stars with good photometry in V and i (sample 1; mean 1 $\sigma$ error bars are given for different i₀ magnitude ranges). A triangle marks the RGB-tip, as we described in Sect. 4.1. The absolute magnitudes are calculated using the distance modulus from Table 1.
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In the text

$\begin{figure} \par\includegraphics[width=16cm,clip]{1045fig3.eps} \end{figure}$ Figure 3: Left: colour-colour diagram for all stars of sample 2. Also plotted are the selection areas for M and C-stars, as described in the text. Right: corresponding colour-magnitude diagram for all stars of sample 2. The identified C-stars from the selection areas, marked with open circles, lie on the uppermost parts of the RGB/AGB-sequences.
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In the text

$\begin{figure} \par\includegraphics[width=17cm,clip]{1045fig4.eps} \end{figure}$ Figure 4: Left: luminosity function (apparent and absolute imagnitude) for the seven C-stars, identified in Fig. 3. Using the distance modulus from Table 1, one can calculate a $\langle$ M_i $\rangle$ . The dotted line marks the RGB-tip from Sect. 4.1. Right: bolometric LFs for all C-stars found. $M_{\rm bol}$ was calculated as described in the text. Note the difference between the mean luminosity $\langle L \rangle$ and the luminosity calculated from the mean $\langle$ $M_{\rm bol}$ $\rangle$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{1045fig5.eps} \end{figure}$ Figure 5: Distribution of all stars of sample 1 on the i-band frame, overplotted are the identified new C-stars (open circles), M-stars (full circles) and the galaxy centre (cross) (see also Sect. 3.2). The line indicates the border of the "foreground'' field in the lower left corner discussed in the text.
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{1045fig6.eps} \end{figure}$ Figure 6: Radial distributions of all stars of sample 1 and for the found C-stars.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1045fig1.eps} \end{figure}$	Figure 1: i-band CCD image of And II obtained at the 2.56 m Nordic Optical Telescope. The field covers $\approx$ 6 $\hbox {$.\mkern -4mu^\prime $ }$ 5 $\times$ 6 $\hbox {$.\mkern -4mu^\prime $ }$ 5, i.e. most of the galaxy with its center somewhat displaced to the upper right. North is up and east to the left.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{1045fig2.eps} \end{figure}$	Figure 2: Colour-magnitude diagrams for the 2307 stars with good photometry in V and i (sample 1; mean 1 $\sigma$ error bars are given for different i₀ magnitude ranges). A triangle marks the RGB-tip, as we described in Sect. 4.1. The absolute magnitudes are calculated using the distance modulus from Table 1.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=16cm,clip]{1045fig3.eps} \end{figure}$	Figure 3: Left: colour-colour diagram for all stars of sample 2. Also plotted are the selection areas for M and C-stars, as described in the text. Right: corresponding colour-magnitude diagram for all stars of sample 2. The identified C-stars from the selection areas, marked with open circles, lie on the uppermost parts of the RGB/AGB-sequences.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{1045fig5.eps} \end{figure}$	Figure 5: Distribution of all stars of sample 1 on the i-band frame, overplotted are the identified new C-stars (open circles), M-stars (full circles) and the galaxy centre (cross) (see also Sect. 3.2). The line indicates the border of the "foreground'' field in the lower left corner discussed in the text.
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$\begin{figure} \par\includegraphics[width=8.7cm,clip]{1045fig6.eps} \end{figure}$	Figure 6: Radial distributions of all stars of sample 1 and for the found C-stars.
Open with DEXTER