Gzipped Postscript Version
Figure 164: in the Ursa Major Cluster.
HI: WSRT, 30'' resolution.
Notes: The following galaxies appear separately within
the Gallery:
NGC3718/29 (Fig. 13);
NGC3769 (Fig. 42);
NGC3893/96 (Fig. 50);
NGC3992 & UGC6923/40/69
(Fig. 181);
NGC4013 (Fig. 15);
NGC4085/88 (Fig. 55);
UGC6962/73 (Fig. 80).
Reference: Verheijen, M. A. W., & Sancisi, R. 2001, A&A,
370, 765. See also Verheijen, these proceedings,
p. 573.
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Figure 165: The Compact Group HCG 90.
HI: VLA D-array, 
resolution,
contours=
cm
.
Optical: DSS, FOV=
.
Notes: All galaxies with known redshifts falling within the
passband of the observations have been labeled.
Reference: Rupen, Hibbard & Bunker, these proceedings,
p. 863.
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Figure 166: The Pegasus I Group.
HI: VLA D-array, 
resolution,
contours=
cm.
Optical: DSS, FOV=
.
Notes: The contours represent the combination of two
separate observations: a pointing centered on
NGC7626 (3423 km s
) which found in the galaxy
UGC12510 and in cloud lying between NGC7626 and NGC7619; and a
separate pointing centered on NGC7617 (4010 km s)
which found everything else.
Reference: Observations centered on NGC7626:
Hibbard & Sansom, these proceedings,
p. 858.
Observations centered on NGC7617: Schiminovich et al., these proceedings,
p. 863.
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Figure 167: The Virgo Cluster near M86.
HI: VLA D-array, 
resolution,
contours=
cm.
Optical: DSS, FOV=
.
Notes: Galaxies labeled in parenthesis have
velocities that fall outside of the observed range.
Reference: Li & van Gorkom, these proceedings,
p. 637.