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Figure 144: The NGC 2964/2968/2970 System.
HI: VLA D-array, resolution,
contours= cm.
Optical: DSS, FOV=.
Notes: This system was targeted because of the presence of
the Type I supernova 1970l that was observed to lie
between NGC2968 and NGC2970.
Reference: Tyson & van Gorkom, these proceedings,
p. 864.
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Figure 145: The Leo Triplet.
HI: Arecibo single dish map.
Contours=(3, 5, 10, 15, 25, 50, 75, 100, 200, 400, 600) K km
s.
Optical: DSS, FOV=.
Reference: Haynes, M. P., Giovanelli, R., Roberts, M.S. 1979,
ApJ, 229, 83.
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Figure 146: The Leo Triplet Member NGC3628.
HI: VLA D-array, 60'' resolution,
contours= cm.
Optical: Top two panels: DSS, FOV=.
Third panel: DSS, FOV=. Bottom panel:
Palomar 48'' Schmidt (B) second blue survey with
high-contrast development by James Schombert, FOV=.
Notes: The dotted boxes in the third panel delineates the
regions shown in the other panels.
Reference: Appleton & Hughes, these proceedings,
p. 856.
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Figure 147: The Ring Galaxy System Arp 141.
HI: VLA B+C+D-array, resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Higdon et al., these proceedings,
p. 859.
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Figure 148: The NGC 5915/6 System.
HI: VLA D-array, 60'' resolution,
contours= cm.
Optical: DSS, FOV=.
Reference: Hameed & Young, these proceedings,
p. 857.
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Figure 149: The Arp 314 System.
HI: VLA D-array, 72'' resolution,
contours= cm.
Optical: Palomar 5m Gunn r, FOV=.
Reference: Nordgren, T. E., Chengalur, J. N., Salpeter,
E. E., & Terzian, Y. 1997, AJ, 114, 913
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Figure 150: The Arp 313 System.
HI: Lower left panel: WSRT, 30'' resolution,
contours= cm. Lower right panel: VLA
D-array, resolution.
Optical: DSS, FOV=.
Notes: The dotted outline in the lower left panel
delineates the region shown in the other panels.
Reference: WSRT observations: Swaters, R. A., 1999, PhD
thesis, Rijksuniversiteit Groningen, and Swaters,
R.A., van Albada, T.S., van der Hulst, J.M., &
Sancisi, R., 2001, A&AS, submitted. VLA observations:
Wilcots, E.M., & Prescott, M.K., 2001, AJ, submitted.