All Figures

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{f1m6909.eps} \end{figure}$ Figure 1: Illustration of the apparent radial velocity distribution on a stellar disk for solid body rotation: vertical lines of constant radial velocity are labeled by their velocity in units of $\ensuremath{V\sin(i)}$ . They lie parallel to rotational pole - disk center direction. For further explanations see text.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{f2m6909.eps} \end{figure}$ Figure 2: Rotationally broadened line profiles (solid lines) for different total numbers of asterocentric angles $\ensuremath {N_\mu }$ employing the broadening procedure of Dravins & Nordlund in comparison to the exact profile (diamonds). For clarity, the broadened line profiles have been vertically offset. Wavelengths are given as Doppler velocities in units of the width of the Gaussian non-broadened profile (dash-dotted line).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{f3m6909.eps} \end{figure}$ Figure 3: As for Fig. 2 for our broadening procedure.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{f4m6909.eps} \end{figure}$ Figure 4: Comparison of rotational broadening assuming a rigidly (solid line) and differentially (diamonds) rotating Sun. Thirty times enlarged differences of the resulting profiles (in the sense differential-rigid) are plotted in the lower part of the panel. For further explanations see text.
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{f1m6909.eps} \end{figure}$	Figure 1: Illustration of the apparent radial velocity distribution on a stellar disk for solid body rotation: vertical lines of constant radial velocity are labeled by their velocity in units of $\ensuremath{V\sin(i)}$ . They lie parallel to rotational pole - disk center direction. For further explanations see text.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{f3m6909.eps} \end{figure}$	Figure 3: As for Fig. 2 for our broadening procedure.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{f4m6909.eps} \end{figure}$	Figure 4: Comparison of rotational broadening assuming a rigidly (solid line) and differentially (diamonds) rotating Sun. Thirty times enlarged differences of the resulting profiles (in the sense differential-rigid) are plotted in the lower part of the panel. For further explanations see text.
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