Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=17.3cm,clip]{0624fig1.eps}\end{figure}$ Figure 1: Histograms of the three sigma standard deviations of all mean photometric values for the programme clusters; arrows indicate the bona-fide variable stars detected.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.5cm,clip]{0624fig2.eps}\end{figure}$ Figure 2: The Hertzsprung-Russell diagram of the variable objects with the parameters listed in Table 2. The zero age main sequence is taken from Schmidt-Kaler (1982). The areas of different variable groups are indicated.
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In the text

$\begin{figure} \par\includegraphics[width=17.3cm,clip]{0624fig1.eps}\end{figure}$	Figure 1: Histograms of the three sigma standard deviations of all mean photometric values for the programme clusters; arrows indicate the bona-fide variable stars detected.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=270,width=8.5cm,clip]{0624fig2.eps}\end{figure}$	Figure 2: The Hertzsprung-Russell diagram of the variable objects with the parameters listed in Table 2. The zero age main sequence is taken from Schmidt-Kaler (1982). The areas of different variable groups are indicated.
Open with DEXTER