Gzipped Postscript Version
Figure 112: The NGC7135 System.
HI: VLA C+D-array, 
resolution,
contours=
cm
.
Optical: DSS, FOV=
.
Reference: Schiminovich et al., these proceedings,
p. 863.
Gzipped Postscript Version
Figure 113: The NGC5018 System.
HI: VLA D-array, 60'' resolution,
contours=
cm.
Optical: DSS, FOV=
.
Reference: Kim, D. -W., Guhathakurta, P., van Gorkom, J. H.,
Jura, M., & Knapp, G. R. 1988, ApJ, 330, 684.
Gzipped Postscript Version
Figure 114: The Arp 227 Shell System.
HI: VLA D-array, 
resolution,
contours=
cm.
Optical: DSS, FOV=
.
Notes: The lower right panel shows an expanded field of
view, showing an detected companion to the south. The dotted box
shows the region imaged in the other three panels.
Reference: Schiminovich et al., these proceedings,
p. 863.
Gzipped Postscript Version
Figure 115: The Fornax A System.
HI: VLA DnC-array, 
resolution,
contours= cm.
Optical: DSS, FOV=
.
Reference: Horellou, C., Black, J. H., van Gorkom, J. H.,
Combes, F., van der Hulst, J. M., & Charmandaris, V. 2001, A&A,
submitted.
Gzipped Postscript Version
Figure 116: The Peculiar Elliptical NGC 4125.
HI: VLA D-array, 
resolution,
contours= cm.
Optical: DSS, FOV=
.
Reference: Rupen, Hibbard & Bunker, these proceedings,
p. 863.
Gzipped Postscript Version
Figure 117: The NGC 7619/7626 System.
HI: VLA D-array, 
resolution,
contours= cm.
Optical: DSS, FOV=
.
Notes: The central galaxies of the Pegasus I group in the
Pegasus Cluster -- see also Fig. 166.
Reference: Observations centered on NGC7626:
Hibbard & Sansom, these proceedings, p. 858.
Observations centered on NGC7617: Schiminovich et al.,
these proceedings, p. 863.
Gzipped Postscript Version
Figure 118: The M86 Region.
HI: VLA D-array, 
resolution,
contours= cm.
Optical: DSS, FOV=
.
Notes: Member of the Virgo cluster. See also
Fig. 167.
Reference: Li & van Gorkom, these proceedings,
p. 637.
Gzipped Postscript Version
Figure 119: The M85 System.
HI: VLA D-array, resolution,
contours= cm.
Optical: DSS, FOV=
.
Reference: Hibbard & Sansom, these proceedings,
p. 858.
Gzipped Postscript Version
Figure 120: Peculiar Early Types Undetected in .
HI:
upper limits are in the range of a few 
.
See Sansom, A.E., Hibbard, J.E., & Schweizer, F., 2001, AJ,
120, 1946.
Optical: DSS.
Notes: For each system, the value of the Fine Structure Index
(FSI), a quantitative measure of optical morphological peculiarity, is
listed. See
Schweizer, F., & Seitzer, P. 1992, AJ, 104, 1039.
Reference: NGC3610, NGC3640 and NGC5322:
Hibbard & Sansom, these proceedings, p. 858.
NGC596, NGC7585 and NGC7600:
Schiminovich et al., these proceedings, p. 863.