$\begin{figure} {\hbox{ \psfig{figure=0937f1a.ps,width=8cm,angle=-90,clip=t} }} {... ...}} {\hbox{ \psfig{figure=0937f1c.ps,width=8cm,angle=-90,clip=t} }}\end{figure}$ Figure 1: Example for the correction of the curvature of the spectra in y-direction. Top: the raw but cosmic corrected two dimensional spectrum of the galaxy A18 (slit No. 18 of setup A) of MS 1008-12. Center: the same spectrum after applying the rectification. Bottom: the fully reduced and wavelength calibrated spectrum. A18 is an early-type galaxy and a member of MS 1008-12 (z=0.3111). Please note that the figures are expanded in y-direction for a better illustration of the curvature.
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In the text

$\begin{figure} {\hbox{ \psfig{figure=0937f2a.ps,width=3.5cm,clip=t}\psfig{figure... ...,angle=-90,clip=t}\psfig{figure=0937f2c.ps,width=5.5cm,clip=t} }} \end{figure}$ Figure 2: Illustration of our observed data by means of one galaxy from Setup B of the cluster MS 1008-12 (ID = B5). Left: the spatially resolved $H_{\beta }$ -emission line showing clearly the Doppler shifts due to the rotation of the galaxy (for a better illustration the image was expanded in the spatial direction). Center: the corresponding measured rotation curve. Right: image of the galaxy extracted from the FORS frame. The galaxy with R=20.70 has an inclination of 60 $^{\circ }$ and is a cluster member (z=0.3039). The slit position is marked.
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In the text

$\begin{figure} {\hbox{ \psfig{figure=0937f3a.ps,width=7cm,height=7cm,clip=t}\psf... ...cm,clip=t}\psfig{figure=0937f3f.ps,width=7cm,height=7cm,clip=t} }}\end{figure}$ Figure 3: Finding charts of all MOS setups. Top: MS 1008-12. Center: Cl 0303+17. Bottom: Cl 0413-65. In all cases we show the full FORS 6 $.\mkern -4mu^\prime$ 8 $\times$ 6 $.\mkern -4mu^\prime$ 8 -FOV. All primary MOS-targets are marked by circles and labeled by their slit numbers. The central cluster galaxy is marked by a square (north is up, east to the left).
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In the text

$\begin{figure} \par\includegraphics[width=14cm,clip]{0937f4.eps} \end{figure}$ Figure 4: Position velocity diagrams of galaxies in the field of MS 1008-12. Galaxies which entered the TF diagram presented in Paper I are labeled (TF). The solid line represents the projected best fitting model profile. See Tables 6-8 for comparison.
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In the text

$\begin{figure} \par\includegraphics[width=13cm,clip]{0937f5.eps} \end{figure}$ Figure 5: Position velocity diagrams of galaxies in the field of Cl 0303+17. Galaxies which entered the TF diagram presented in Paper I are labeled (TF). The solid line represents the projected best fitting model profile. See Table 9 for comparison.
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In the text

$\begin{figure} \par\includegraphics[width=13cm,clip]{0937f6.eps} \end{figure}$ Figure 6: Position velocity diagrams of galaxies in the field of Cl 0413-65. Galaxies which entered the TF diagram presented in Paper I are labeled (TF). The solid line represents the projected best fitting model profile. See Tables 10 and 11 for comparison.
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In the text

$\begin{figure} {\hbox{ \psfig{figure=0937f3a.ps,width=7cm,height=7cm,clip=t}\psf... ...cm,clip=t}\psfig{figure=0937f3f.ps,width=7cm,height=7cm,clip=t} }}\end{figure}$	Figure 3: Finding charts of all MOS setups. Top: MS 1008-12. Center: Cl 0303+17. Bottom: Cl 0413-65. In all cases we show the full FORS 6 $.\mkern -4mu^\prime$ 8 $\times$ 6 $.\mkern -4mu^\prime$ 8 -FOV. All primary MOS-targets are marked by circles and labeled by their slit numbers. The central cluster galaxy is marked by a square (north is up, east to the left).
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$\begin{figure} \par\includegraphics[width=14cm,clip]{0937f4.eps} \end{figure}$	Figure 4: Position velocity diagrams of galaxies in the field of MS 1008-12. Galaxies which entered the TF diagram presented in Paper I are labeled (TF). The solid line represents the projected best fitting model profile. See Tables 6-8 for comparison.
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$\begin{figure} \par\includegraphics[width=13cm,clip]{0937f5.eps} \end{figure}$	Figure 5: Position velocity diagrams of galaxies in the field of Cl 0303+17. Galaxies which entered the TF diagram presented in Paper I are labeled (TF). The solid line represents the projected best fitting model profile. See Table 9 for comparison.
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$\begin{figure} \par\includegraphics[width=13cm,clip]{0937f6.eps} \end{figure}$	Figure 6: Position velocity diagrams of galaxies in the field of Cl 0413-65. Galaxies which entered the TF diagram presented in Paper I are labeled (TF). The solid line represents the projected best fitting model profile. See Tables 10 and 11 for comparison.
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