Gzipped Postscript Version
Figure 95: The Ring Galaxy System AM 1354-250.
HI: VLA CnB+DnC-array, resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Higdon et al., these proceedings,
p. 859.
Gzipped Postscript Version
Figure 96: The Ring Galaxy System Arp 147.
HI: VLA B-array, resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Higdon et al., these proceedings,
p. 859.
Gzipped Postscript Version
Figure 97: The Lindsay-Shapley Ring.
HI: ATCA, resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Higdon et al., these proceedings,
p. 859.
Gzipped Postscript Version
Figure 98: The NGC 2292/3 system.
HI: VLA D-array, resolution,
contours= cm.
Optical: DSS, FOV= and .
Notes: No was detected from NGC 2295 or ESO 490-GO42,
even though they have velocities within the range of the \
observations.
Reference: Rupen, Hibbard & Bunker, these proceedings,
p. 863.
Gzipped Postscript Version
Figure 99: The NGC5506/7 System.
HI: VLA C-array, resolution,
contours= cm.
Optical: DSS, FOV=.
Notes: A lower resolution map of this system showing more
widely distributed gas is shown in Fig. 151.
Reference: Mundell, these proceedings,
p. 411.
Gzipped Postscript Version
Figure 100: The Arp 102 System.
HI: VLA D-array, 52'' resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Higdon et al., these proceedings,
p. 859.
Gzipped Postscript Version
Figure 101: The Arp 104 System.
HI: VLA D-array, 52'' resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Higdon et al., these proceedings,
p. 859.
Gzipped Postscript Version
Figure 102: The Arp 105 System.
HI: VLA C+D-array, resolution,
contours= cm.
Optical: CFHT 4m V-band, FOV=.
Notes: In the cluster Abell 1185.
Reference: Duc, P. -A., Brinks, E., Wink, J. E., &
Mirabel, I. F. 1997, A&A, 326, 537.
Gzipped Postscript Version
Figure 103: The Ring Galaxy NGC2444/5.
HI: VLA C+D-array, 28'' resolution,
contours= cm.
Optical: KPNO 0.9m B-band, FOV=.
Reference: Appleton, P. N., Ghigo, F. D, van Gorkom, J. H.,
Schombert, J. M., & Struck-Marcell, C. 1987, Nature, 330, 140.
Gzipped Postscript Version
Figure 104: The Arp 94 System.
HI: VLA D-array, resolution,
contours= cm.
Optical: DSS, FOV= (left) and
(right).
Reference: Mundell, these proceedings,
p. 411.
Gzipped Postscript Version
Figure 105: The IR luminous merger Mrk 273.
HI: VLA CnB-array, resolution,
contours= cm.
Optical: Lower Right: DSS, FOV=.
Other: UH 88'' R-band, FOV=.
Notes: was also detected in UGC8707 and the companion
to the north.
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 106: The Toomre Sequence merger NGC3921.
HI: VLA C+D-array, 20'' resolution,
contours= cm.
Optical: KPNO 2.1m R-band, FOV= (top),
(bottom).
Notes: MCG+09-19-213 falls on the edge of the passband
of the observations, so is not completely mapped in HI.
Reference: Hibbard, J. E., & van Gorkom, J. H. 1996, AJ,
111, 655.