All Figures

$\begin{figure} \par\includegraphics[width=17.2cm,clip]{8119fig1.ps} \end{figure}$ Figure 1: Field containing 11 of the 12 confirmed members of the NGC 4410 group. Letters from A to H, and K refer to NGC 4410A, NGC 4410B, etc. (FGC 170A, the 12th confirmed member, lies to the north of this field). The naming of the group members is as used in Smith (2000). NGC 4410A has coordinates $\alpha =\rm 12^{h}23^{m}55^{s}$ , $\delta = 09^{\circ }17'40''$ (J2000.0). The directions North and East are indicated. The image is part of the co-addition of digital scans of 13 Kodak Tech-Pan Schmidt films (Katsiyannis et al. 1998).
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{8119fig2.ps} \end{figure}$ Figure 2: A high contrast image of the four interacting components in the NGC 4410 group from the digitally co-added Schmidt Tech-Pan films.
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{8119fig3.ps} \end{figure}$ Figure 3: A skewness representation of the NGC 4410 group showing the extent of faint diffuse matter.
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In the text

$\begin{figure} \par\includegraphics[width=14.5cm,clip]{8119fig4.ps} \end{figure}$ Figure 4: Residual images of the galaxy group components NGC 4410A, C, D from B images from: a) the 2.1 m telescope; b) the Jacobus Kapteyn (1 m) Telescope; c) the 0.84 m telescope; and d) a residual B image of NGC 4410B,C,D from the 1 m JKT telescope. The residual image of NGC 4410A shows possible ``spiral arm-like'' asymmetrical structures near the nucleus. NGC 4410D shows a prominent bar distorted by the group interaction in all four images.
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig5.ps} \end{figure}$ Figure 5: a) NGC 4410A/B in a logarithmic image; b) a (B-V) color map image; c) a B residual image of NGC 4410A from the 2.1 m telescope; d) a B residual image of NGC 4410A from the 0.84 m telescope, in which spiral arms seem to be coincident with some of the H II regions found in this galaxy; e) a processed HST public image shows the residual structure of the nucleus of NGC 4410A; f) an unsharp masked image in B from the 2.1 m telescope; g) the (H $\alpha + [$ N II]) image of NGC 4410A/B from Donahue et al. (2002); h) our (H $\alpha + [$ N II]) image from the 2.1 m telescope.
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig6.eps} \end{figure}$ Figure 6: Surface brightness and color profiles of NGC 4410A a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig7.ps} \end{figure}$ Figure 7: Residual images of NGC 4410B in B band, a) 2.1 m telescope, b) 1 m telescope, c) 0.84 m telescope.
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig8.eps} \end{figure}$ Figure 8: Surface brightness and color profiles of NGC 4410B a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig9.eps} \end{figure}$ Figure 9: Position angle versus radius profiles for a) NGC 4410A, b) NGC 4410B, c) NGC 4410C, and d) NGC 4410D from the 2.1 m telescope in B band. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg10.eps} \end{figure}$ Figure 10: Profiles of the a₄/a harmonic term versus radius for a) NGC 4410A, b) NGC 4410B, c) NGC 4410C, and d) NGC 4410D from the 2.1 m telescope in B band. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg11.ps} \end{figure}$ Figure 11: NGC 4410C in a) a logarithmic image in B, b) a (B-V) color map image, c) a residual image, and d) an unsharp masked image from the 2.1 m telescope. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg12.eps} \end{figure}$ Figure 12: Surface brightness and color profiles of NGC 4410C a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg13.ps} \end{figure}$ Figure 13: NGC 4410D in a) a logarithmic image in B, b) a (B-V) color map image, c) a residual image in B, d) an unsharp masked image, e) (H $\alpha + [$ N II]) image, all from the 2.1 m telescope. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg14.eps} \end{figure}$ Figure 14: Surface brightness and color profiles of NGC 4410D a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{8119fig2.ps} \end{figure}$	Figure 2: A high contrast image of the four interacting components in the NGC 4410 group from the digitally co-added Schmidt Tech-Pan films.
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$\begin{figure} \par\includegraphics[width=6.8cm,clip]{8119fig3.ps} \end{figure}$	Figure 3: A skewness representation of the NGC 4410 group showing the extent of faint diffuse matter.
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig6.eps} \end{figure}$	Figure 6: Surface brightness and color profiles of NGC 4410A a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig7.ps} \end{figure}$	Figure 7: Residual images of NGC 4410B in B band, a) 2.1 m telescope, b) 1 m telescope, c) 0.84 m telescope.
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig8.eps} \end{figure}$	Figure 8: Surface brightness and color profiles of NGC 4410B a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fig9.eps} \end{figure}$	Figure 9: Position angle versus radius profiles for a) NGC 4410A, b) NGC 4410B, c) NGC 4410C, and d) NGC 4410D from the 2.1 m telescope in B band. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg10.eps} \end{figure}$	Figure 10: Profiles of the a₄/a harmonic term versus radius for a) NGC 4410A, b) NGC 4410B, c) NGC 4410C, and d) NGC 4410D from the 2.1 m telescope in B band. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg11.ps} \end{figure}$	Figure 11: NGC 4410C in a) a logarithmic image in B, b) a (B-V) color map image, c) a residual image, and d) an unsharp masked image from the 2.1 m telescope. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg12.eps} \end{figure}$	Figure 12: Surface brightness and color profiles of NGC 4410C a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg13.ps} \end{figure}$	Figure 13: NGC 4410D in a) a logarithmic image in B, b) a (B-V) color map image, c) a residual image in B, d) an unsharp masked image, e) (H $\alpha + [$ N II]) image, all from the 2.1 m telescope. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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$\begin{figure} \par\includegraphics[width=12cm,clip]{8119fg14.eps} \end{figure}$	Figure 14: Surface brightness and color profiles of NGC 4410D a) V, b) B-V, c) V-R, and d) V-I. (1''= 470 pc with H₀= 75 km s^-1 Mpc^-1).
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