All Figures

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315fig1.ps}} \end{figure}$ Figure 1: A small region of the non-normalized spectra of $\gamma$ Boo (grey) and HD 118623 (black). The fit to the assumed continuum is overplotted and is in good agreement with both spectra.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315fig2.ps}} \end{figure}$ Figure 2: Normalized spectra of HD 118623 (grey) and Altair (black). The whole region used to derive Altair's broadening function is shown.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315fig3.ps}} \end{figure}$ Figure 3: Comparison of the normalized spectra of HD 27819 (grey line) and Altair (black line) in a small spectral window.
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In the text

$\begin{figure} \includegraphics[height=16cm,width=7cm,angle=-90,clip=]{HD27819_f... ...ight=5.2cm,width=2.5cm,angle=-90,clip=]{1315fig4.ps}\vspace{3.4cm}\end{figure}$ Figure 4: Data (grey) and fit (black) achieved from our deconvolution algorithm for HD 27819. The quality of the fit is typical for the whole wavelength region. The deconvolved "global'' profile is plotted in the inset.
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In the text

$\begin{figure} \includegraphics[height=16cm,width=7cm,angle=-90,clip=]{Altair_fi... ...ht=5.2cm,width=2.5cm,angle=-90,clip=]{1315fig5.ps} \vspace{3.4cm} \end{figure}$ Figure 5: Data (grey line) and achieved fit (black line) of Altair. Fit quality is typical for the whole wavelength region. The deconvolved "overall'' profile is plotted in the inset.
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In the text

$\begin{figure} \mbox{ \resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{131... ...esizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315f6b.ps}} }\end{figure}$ Figure 6: Left panel: global broadening function of Altair reconstructed from about 650 lines. Error bars corresponding to a signal-to-noise ratio of 1000 are overplotted. Right panel: Fourier transform of the reconstructed broadening function ( left panel) with its error bars. Note the logarithmic scale on the y-axis.
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In the text

$\begin{figure} \mbox{ \resizebox{8.8cm}{!}{\includegraphics{1315f7a.ps}}\resizebox{8.8cm}{!}{\includegraphics{1315f7b.ps}} } \end{figure}$ Figure 7: Left panel: equatorial velocity v as a function of q₂/q₁ according to Eq. (1). Vertical lines indicate measured values of q₂/q₁ and its confidence levels, the horizontal line shows the measured $v~\sin{i}$ . The allowed region where $v > v~\sin{i}$ is plotted as a thick line. Right panel: inclination angle i (in degree) of Altair as function of q₂/q₁ (solid thick line). Measurements of q₂/q₁ are plotted as in the left panel. Dashed lines indicate the region allowed taking into account the systematic errors of $v~\sin{i}$ .
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315fig1.ps}} \end{figure}$	Figure 1: A small region of the non-normalized spectra of $\gamma$ Boo (grey) and HD 118623 (black). The fit to the assumed continuum is overplotted and is in good agreement with both spectra.
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$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315fig2.ps}} \end{figure}$	Figure 2: Normalized spectra of HD 118623 (grey) and Altair (black). The whole region used to derive Altair's broadening function is shown.
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$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315fig3.ps}} \end{figure}$	Figure 3: Comparison of the normalized spectra of HD 27819 (grey line) and Altair (black line) in a small spectral window.
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$\begin{figure} \includegraphics[height=16cm,width=7cm,angle=-90,clip=]{HD27819_f... ...ight=5.2cm,width=2.5cm,angle=-90,clip=]{1315fig4.ps}\vspace{3.4cm}\end{figure}$	Figure 4: Data (grey) and fit (black) achieved from our deconvolution algorithm for HD 27819. The quality of the fit is typical for the whole wavelength region. The deconvolved "global'' profile is plotted in the inset.
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$\begin{figure} \includegraphics[height=16cm,width=7cm,angle=-90,clip=]{Altair_fi... ...ht=5.2cm,width=2.5cm,angle=-90,clip=]{1315fig5.ps} \vspace{3.4cm} \end{figure}$	Figure 5: Data (grey line) and achieved fit (black line) of Altair. Fit quality is typical for the whole wavelength region. The deconvolved "overall'' profile is plotted in the inset.
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$\begin{figure} \mbox{ \resizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{131... ...esizebox{8.8cm}{!}{\includegraphics[angle=-90,clip]{1315f6b.ps}} }\end{figure}$	Figure 6: Left panel: global broadening function of Altair reconstructed from about 650 lines. Error bars corresponding to a signal-to-noise ratio of 1000 are overplotted. Right panel: Fourier transform of the reconstructed broadening function ( left panel) with its error bars. Note the logarithmic scale on the y-axis.
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