$\begin{figure} \par\includegraphics[width=11cm,clip]{0171fig1.ps}\end{figure}$ Figure 1: The discrete Fourier transform of the integrated RV measurements for each of the nights of our observations. The vertical dashed lines mark the frequencies of the known photometric modes.
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In the text

$\begin{figure} \par\includegraphics[width=15cm,clip]{0171fig2.ps}\end{figure}$ Figure 2: The spectral region of 10 Aql near the high amplitude RV lines which are marked by vertical lines.
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In the text

$\begin{figure} \par\includegraphics[width=11cm,clip]{0171fig3.ps}\end{figure}$ Figure 3: The discrete Fourier transform for the spectral lines showing evidence for pulsational RV variations for the three nights of our observations. Each night is shown in vertical panels. The number in the upper right corner of each panel is the wavelength of the spectral line in Å.
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In the text

$\begin{figure} \par\includegraphics[width=15cm]{0171fig4.ps}\end{figure}$ Figure 4: The radial velocity variations for the 5471.40 Å feature on the night of 11 Aug. 1998.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0171fig5.ps}\end{figure}$ Figure 5: The radial velocity variations for the $\lambda$ 5471.40 Å feature on the night of 11 Aug. 1998 phased to the pulsation period of 11.54 min (filled circles). The values are repeated for the second cycle (open circles).
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In the text

$\begin{figure} \par\includegraphics[width=11cm,clip]{0171fig1.ps}\end{figure}$	Figure 1: The discrete Fourier transform of the integrated RV measurements for each of the nights of our observations. The vertical dashed lines mark the frequencies of the known photometric modes.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15cm,clip]{0171fig2.ps}\end{figure}$	Figure 2: The spectral region of 10 Aql near the high amplitude RV lines which are marked by vertical lines.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=11cm,clip]{0171fig3.ps}\end{figure}$	Figure 3: The discrete Fourier transform for the spectral lines showing evidence for pulsational RV variations for the three nights of our observations. Each night is shown in vertical panels. The number in the upper right corner of each panel is the wavelength of the spectral line in Å.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15cm]{0171fig4.ps}\end{figure}$	Figure 4: The radial velocity variations for the 5471.40 Å feature on the night of 11 Aug. 1998.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{0171fig5.ps}\end{figure}$	Figure 5: The radial velocity variations for the $\lambda$ 5471.40 Å feature on the night of 11 Aug. 1998 phased to the pulsation period of 11.54 min (filled circles). The values are repeated for the second cycle (open circles).
Open with DEXTER