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Figure 73: The Large and Small Magellanic Clouds and the
Magellanic Stream.
HI: Parkes Multibeam All-Sky Survey (see Stavely-Smith et
al., these proceedings, p. 427), 15.5' resolution,
contours= cm.
Optical: Image from the color imaging team
at Mt. Stromlo Observatory (see Bessell, M. 2000, PASA, 17, 179).
Reference: Putman, M.E., et al., 1998, Nature, 394, 752.
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Figure 74: The NGC 7769/7771 System.
HI: VLA D-array, resolution,
contours= cm.
Optical: Top panels: Palomar 5m Gunn r, FOV=.
Bottom left panel: DSS, FOV=.
Reference: Nordgren, T. E., Chengalur, J. N., Salpeter,
E. E., & Terzian, Y. 1997, AJ, 114, 77.
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Figure 75: The Arp 270 System.
HI: VLA C+D-array, 21'' resolution,
contours= cm.
Optical: DSS, FOV= (top),
(bottom).
Reference: Clemens, M. S., Baxter, K. M., Alexander, P.,
& Green, D. A. 1999, MNRAS, 308, 364. See also Clemens, Winter, &
Alexander, these proceedings, p. 208.
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Figure 76: The IR Luminous Merger NGC 6670.
HI: VLA C-array, resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Wang, W.-H., Lo, K. Y., Gao, Y., & Gruendl, R. A. 2001,
AJ, 121, 140.
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Figure 77: The IR luminous merger Arp 299.
HI: VLA C+D-array.
Lower left: 21'' resolution, contours=
cm.
Lower right: 35'' resolution.
Optical: UH 88'' B-band, FOV=.
Notes: There is a small detected companion 10' to
the west of Arp 299.
Reference: Hibbard, J. E., & Yun, M. S. 1999, AJ, 118, 162.
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Figure 78: The IR luminous merger NGC1614.
HI: VLA C+D-array, 19'' resolution,
contours= cm.
Optical: UH 88'' B-band, FOV= (top),
(bottom left).
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.