)
Gzipped Postscript Version
Figure 62: The NGC 5713/5719 System.
HI: VLA C-array, 30'' resolution,
contours=
cm
.
Optical: DSS, FOV=
.
Reference: Langston & Teuben, these proceedings,
p. 861.
Gzipped Postscript Version
Figure 63: The NGC 7714/15 System.
HI: VLA B+C+D-array, 
resolution,
contours=
cm.
Optical: DSS, FOV=
.
Reference: Smith, B.J. 1991, ApJ, 393, 544 and
Smith, B.J., Struck, C., & Pogge, R.W. 1997, ApJ,
483, 754.
Gzipped Postscript Version
Figure 64: The Arp 245 System.
HI: VLA CS-array, 25'' resolution,
contours=
cm.
Optical: Top: NTT+CFHT V-band. Bottom left: DSS.
FOV=
.
Reference: Duc, P. -A., Brinks, E., Springel, V., Pichardo,
B., Weilbacher, P., & Mirabel, I.F., 2000, AJ, 120, 1238.
Gzipped Postscript Version
Figure 65: The Toomre Sequence merger NGC4038/9.
HI: VLA C+D-array, 40'' resolution,
contours=
cm.
Optical: DSS, FOV=
.
Notes: The concentration at the end of the southern tail
is associated with a putative Tidal Dwarf Galaxy. For a close-up of
the companion galaxy ESO 572-G045 see Fig. 22.
Reference: Hibbard, J.E., van der Hulst,
J. M., Barnes, J. E., & Rich, R. M. 2001, AJ, in press.
Gzipped Postscript Version
Figure 66: The Toomre Sequence merger NGC4676.
HI: VLA C+D-array, 12'' resolution,
contours= cm.
Optical: KPNO 2.1m B-band, FOV=
.
Notes: There is an detected companion lying 12.8' to
the south (NGC4676S) with no optical counterpart visible on the DSS.
Reference: Hibbard, J. E. & van Gorkom, J. H. 1996, AJ, 111, 655.
Gzipped Postscript Version
Figure 67: The Arp 263 System.
HI: VLA D-array, 
resolution,
contours=
cm.
Optical: DSS, FOV=
.
Notes: The galaxies marked in parenthesis have
redshifts which place them in the background. CGCG 094-040 has no
known redshift.
Reference: Iyer et al., these proceedings,
p. 860.
Gzipped Postscript Version
Figure 68: The NGC1487 System.
HI: ATCA, 17'' resolution,
contours= cm.
Optical: DSS, FOV=
.
Reference: English & Freeman, these proceedings,
p. 857.
Gzipped Postscript Version
Figure 69: The IR luminous Toomre Sequence merger NGC 2623.
HI: VLA C+D-array. Middle panel: 16'' resolution,
contours= cm. Bottom panel: 21''
resolution, contours=
cm.
Optical: Top and middle panels: UH 88'' R-band,
FOV=
. Bottom panel: DSS, FOV=
.
Reference: Hibbard, J.E., & Yun, M. S. 1996,
in Cold Gas at High Redshift, eds. M. Bremer, H. Rottgering,
P. van der Werf, & C. L. Carilli (Dordrecht: Kluwer), 47.
Gzipped Postscript Version
Figure 70: The Toomre Sequence merger NGC3256.
HI: ATCA, 22.6'' resolution,
contours=(2.2, 3.2, 4.3, 22, 43) 
cm
.
Optical: Top panel: UH 88'' R-band.
Bottom panel: DSS, FOV=
.
Notes: The nearby galaxies NGC 3256C, NGC 3262 and
NGC 3263 were also detected in as part of these observations.
Reference: English, J., Norris, R. P., Freeman, K. C., &
Booth, R. S. 2001, AJ, in press.
Gzipped Postscript Version
Figure 71: The IR luminous merger Arp 193.
HI: VLA C+D-array, 
resolution,
contours=
cm.
Optical: UH 88'' B-band, FOV=
.
Reference: Hibbard, J.E., & Yun, M. S. 1996,
in Cold Gas at High Redshift, eds. M. Bremer, H. Rottgering,
P. van der Werf, & C. L. Carilli (Dordrecht: Kluwer), 47.
Gzipped Postscript Version
Figure 72: The Toomre Sequence merger NGC7252.
HI: VLA C+D-array, 
resolution,
contours= cm.
Optical: DSS, FOV=
(top panels) and
CTIO 4m R-band, FOV= 
(bottom panels).
Notes: The bright clump in the northwest tail is
associated with a putative Tidal Dwarf Galaxy.
Reference: Hibbard, J.E., Guhathakurta, P., van Gorkom, J. H.,
& Schweizer, F. 1994, AJ, 107, 67.