Up: The influence of interactions disks

7 Fig. 4 and 5

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Figure 4: Optical (R, r) and near infrared (H, K', K) contour maps of the sample of interacting/merging galaxies studied in this paper (see Table 4). The contour interval is 0.4 mag, starting at a faintest level of 0.5 mag above the noise level of the corresponding image

$\begin{figure}{\begin{tabular}{cc} \vspace{-2.0cm} \includegraphics[clip,height=... ...& \includegraphics[clip,height=50mm]{e357_26.ps}\end{tabular}}\par\end{figure}$

Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 4: continued

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Figure 5: Optical (R, r) and near infrared (H, K', K) contour maps of the sample of non-interacting galaxies studied in this paper (see Table 4). The contour interval is 0.4 mag, starting at a faintest level of 0.5 mag above the noise level of the corresponding image

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

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Figure 5: continued

Up: The influence of interactions disks