All Figures

$\begin{figure} \par\includegraphics[angle=90,width=8.8cm,clip]{H4338F1.PS}\par\vspace*{4mm} \includegraphics[angle=90,width=8.8cm,clip]{H4338F2.PS}\end{figure}$ Figure 1: Blue optical spectra of stars in the region of Bochum 7.
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In the text

$\begin{figure} \par\includegraphics[angle=90, width=8.3cm,clip]{H4338F3.PS}\end{figure}$ Figure 2: A continuum rectified spectrum of LSS 1135 obtained at CASLEO in April 1997 with the instrumental configuration III. Principal spectral features are identified.
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In the text

$\begin{figure} \par\includegraphics[angle=90, width=8.3cm,clip]{H4338F4.PS}\end{figure}$ Figure 3: Radial velocities of LSS 1135 from Table 3 phased with the period of 2.7532 days. Filled circles represent radial velocities measured in spectra observed with the instrumental configuration II, and empty triangles and empty circles those observed with the instrumental configuration I and III, respectively. Continuous curve represents the orbital solution from Table 4.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.8cm,clip]{H4338F1.PS}\par\vspace*{4mm} \includegraphics[angle=90,width=8.8cm,clip]{H4338F2.PS}\end{figure}$	Figure 1: Blue optical spectra of stars in the region of Bochum 7.
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$\begin{figure} \par\includegraphics[angle=90, width=8.3cm,clip]{H4338F3.PS}\end{figure}$	Figure 2: A continuum rectified spectrum of LSS 1135 obtained at CASLEO in April 1997 with the instrumental configuration III. Principal spectral features are identified.
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$\begin{figure} \par\includegraphics[angle=90, width=8.3cm,clip]{H4338F4.PS}\end{figure}$	Figure 3: Radial velocities of LSS 1135 from Table 3 phased with the period of 2.7532 days. Filled circles represent radial velocities measured in spectra observed with the instrumental configuration II, and empty triangles and empty circles those observed with the instrumental configuration I and III, respectively. Continuous curve represents the orbital solution from Table 4.
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