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\@writefile{lof}{\contentsline {figure}{\numberline {1.1}{\ignorespaces The combined, background--subtracted $V$--band image of A3888 from our LCO 100--inch observations. The gray--scale is linear over the range 25--29.5 mag arcsec$^{-2}$.}}{2}}
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\@writefile{lof}{\contentsline {figure}{\numberline {1.2}{\ignorespaces The center of A3888 in $V$ (see Figure 1). The gray--scale is linear over the range 20.4--29.5 mag arcsec$^{-2}$. }}{3}}
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\@writefile{lof}{\contentsline {figure}{\numberline {1.3}{\ignorespaces Two low surface brightness feature from the $V-$band image (Figure 3). The images are plotted with a gray--scale range of 23.7--27.2 mag arcsec$^{-2}$. In the image on the left, a feature which appears to be tidal debris (tails extending up and down) is visible to the left of the compact galaxy near the center. In the image on the right, a very low surface brightness feature extends to the lower right hand corner from the compact galaxy above and left of the center. The nature of both features may be easier to interpret after we have modeled and subtracted the brighter resolved galaxies.}}{4}}
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