Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{0659_fig1.ps} \end{figure}$ Figure 1: Colour Magnitude diagram at observed maximum brightness for the 459 variable stars which have one B measurement.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig2.ps}\end{figure}$ Figure 2: Variable star B030: P= 60 days; R= 20.5.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig3.ps}\end{figure}$ Figure 3: Variable star B098: P= 103 days; R= 21.1.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig4.ps}\end{figure}$ Figure 4: Variable star A266: P= 111 days; R= 21.1.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig5.ps}\end{figure}$ Figure 5: Variable star C128: P= 165 days; R= 20.7.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig6.ps}\end{figure}$ Figure 6: Variable star A185: P= 196 days; R= 20.6.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig7.ps}\end{figure}$ Figure 7: Variable star C004: P= 335 days; R= 19.9.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig8.ps}\end{figure}$ Figure 8: Variable star C169: P= 216 days; R= 21.0.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig9.ps}\end{figure}$ Figure 9: Variable star C072: P= 344 days; R= 20.1.
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In the text

$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig10.ps}\end{figure}$ Figure 10: Variable star A001: P= 368 days; R= 19.5.
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In the text

Fig.2.-Fig.10. Variable light-curves fitted by their Scargle sinusoid. X-axis is in (J-24449624.5) days, Y-axis in ADU/sec. The 3 first objects are of the Cepheid type, the 5 last ones are certainly LPVs.

$\begin{figure} \par\includegraphics[width=6.9cm,clip]{0659_fig11.eps}\end{figure}$ Figure 11: Period Luminosity Diagram: R magnitude is plotted against the period for the stars selected in Table 2. Locations for Cepheids, RV Tauri stars and Miras are shown. Details are given in the text.
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In the text

$\begin{figure} \par\includegraphics[width=15.5cm,clip]{0659_fig12.eps}\end{figure}$ Figure 12: Light curves of the 12 novae candidates detected in the Pic-du Midi AGAPE survey.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{0659_fig1.ps} \end{figure}$	Figure 1: Colour Magnitude diagram at observed maximum brightness for the 459 variable stars which have one B measurement.
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$\begin{figure} \par\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig2.ps}\end{figure}$	Figure 2: Variable star B030: P= 60 days; R= 20.5.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig3.ps}\end{figure}$	Figure 3: Variable star B098: P= 103 days; R= 21.1.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig4.ps}\end{figure}$	Figure 4: Variable star A266: P= 111 days; R= 21.1.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig5.ps}\end{figure}$	Figure 5: Variable star C128: P= 165 days; R= 20.7.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig6.ps}\end{figure}$	Figure 6: Variable star A185: P= 196 days; R= 20.6.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig7.ps}\end{figure}$	Figure 7: Variable star C004: P= 335 days; R= 19.9.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig8.ps}\end{figure}$	Figure 8: Variable star C169: P= 216 days; R= 21.0.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig9.ps}\end{figure}$	Figure 9: Variable star C072: P= 344 days; R= 20.1.
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$\begin{figure}\includegraphics[angle=-90,width=6.55cm,clip]{0659_fig10.ps}\end{figure}$	Figure 10: Variable star A001: P= 368 days; R= 19.5.
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$\begin{figure} \par\includegraphics[width=6.9cm,clip]{0659_fig11.eps}\end{figure}$	Figure 11: Period Luminosity Diagram: R magnitude is plotted against the period for the stars selected in Table 2. Locations for Cepheids, RV Tauri stars and Miras are shown. Details are given in the text.
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{0659_fig12.eps}\end{figure}$	Figure 12: Light curves of the 12 novae candidates detected in the Pic-du Midi AGAPE survey.
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