All Figures

$\begin{figure} \par {\includegraphics[width=8.5cm,clip,angle=0]{0475fig1.ps} }\end{figure}$ Figure 1: The ionized-gas velocity profiles measured along the optical minor axis of NGC 4420 ( $\rm PA = 98^\circ$ , Fisher et al. 1997), NGC 7213 ( $\rm PA = 34^\circ$ , Corsini et al. 2003), NGC 2855 ( $\rm PA = 30^\circ$ , Corsini et al. 2002), NGC 4111 ( $\rm PA = 60^\circ$ , Fisher 1997), and NGC 6810 ( $\rm PA = 86^\circ$ , this paper) are given as prototypical examples for the five classes of minor-axis velocity profiles described in Sect. 2. Errorbars smaller than symbols are not plotted.
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In the text

$\begin{figure} \par {\includegraphics[angle=-90,width=10.24cm,clip]{0475fg2a.ps}... ...udegraphics[height=7.2cm,width=5.65cm,angle=-90,clip]{0475fg2h.ps} \end{figure}$ Figure 2: Ionized-gas kinematics measured along the optical major ( left panels) and minor axes ( right panels) of the 4 sample galaxies. Errorbars smaller than symbols are not plotted.
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In the text

$\begin{figure} \par { \includegraphics[clip=true,width=7.8cm,clip]{0475fg3a.ps}\... ...{2mm} \includegraphics[clip=true,width=7.78cm,clip]{0475fg3d.ps} }\end{figure}$ Figure 3: Surface-brightness ( upper panel), ellipticity ( central panel) and position angle ( lower panel) radial profiles for the sample galaxies. Data for NGC 949, NGC 2460, and NGC 6810 and in H band, data for NGC 2541 are in i band.
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In the text

$\begin{figure} \par { \includegraphics[width=8.5cm,clip=, ]{0475fg4a.ps} } { \includegraphics[width=8.5cm,clip=, ]{0475fg4b.ps} }\end{figure}$ Figure 4: Distribution of the gas velocity gradient along the optical minor axis of the unbarred ( upper panel) and barred ( lower panel) galaxies we collected in Table 1 according to their RSA morphological classification. The white and black regions identify galaxies with (Classes O, C, and G) and without a minor-axis velocity gradient (Class Z), respectively. The shaded region identify galaxies assigned to Class I. The last bins of the panels include all the galaxies with a morphological type later than Sd and SBd, respectively.
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In the text

$\begin{figure} \par {\includegraphics[angle=-90,width=10.24cm,clip]{0475fg2a.ps}... ...udegraphics[height=7.2cm,width=5.65cm,angle=-90,clip]{0475fg2h.ps} \end{figure}$	Figure 2: Ionized-gas kinematics measured along the optical major ( left panels) and minor axes ( right panels) of the 4 sample galaxies. Errorbars smaller than symbols are not plotted.
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$\begin{figure} \par { \includegraphics[clip=true,width=7.8cm,clip]{0475fg3a.ps}\... ...{2mm} \includegraphics[clip=true,width=7.78cm,clip]{0475fg3d.ps} }\end{figure}$	Figure 3: Surface-brightness ( upper panel), ellipticity ( central panel) and position angle ( lower panel) radial profiles for the sample galaxies. Data for NGC 949, NGC 2460, and NGC 6810 and in H band, data for NGC 2541 are in i band.
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