Gzipped Postscript Version
Figure 130: The Polar Ring Galaxy UGC 7576.
HI: VLA C-array, 10'' resolution.
Optical: Top: DSS. Bottom: WIYN V-band image,
FOV=
.
Reference: Cox, A.L., & Sparke, L.S. 1996, ASP Conf.\
Ser. 106, The Minnesota Lectures on Extragalactic Neutral Hydrogen,
ed. E.D. Skillman (ASP, SF), 168.
Gzipped Postscript Version
Figure 131: The IC2006 System.
HI: VLA D-array, 40'' resolution,
contours=
cm
.
Optical: DSS, FOV=
.
Reference: Franx, M., van Gorkom, J. H., & de Zeeuw, P. T.
1994, ApJ, 436, 642 and Schweizer, F., van Gorkom, J. H., & Seitzer,
P. 1989, ApJ, 338, 770.
Gzipped Postscript Version
Figure 132: The NGC 2810 System.
HI: VLA D-array, 
resolution,
contours=
cm.
Optical: DSS, FOV=
(top),
(bottom).
Reference: Schiminovich et al., these proceedings,
p. 863.
Gzipped Postscript Version
Figure 133: The NGC 2768 System.
HI: VLA D-array, 
resolution,
contours= cm.
Optical: DSS, FOV=
.
Reference: Schiminovich et al., these proceedings,
p. 863.
Gzipped Postscript Version
Figure 134: The NGC4026 System.
HI: VLA D-array, 45'' resolution,
contours= cm.
Optical: DSS, FOV=
.
Notes: One of the three brightest lenticulars in the Ursa
Major cluster, all of which show disturbed HI.
Reference: Verheijen & Zwaan, these proceedings,
p. 866.
Gzipped Postscript Version
Figure 135: The NGC 3998 System.
HI: VLA D-array, 45'' resolution,
contours= cm.
Optical: DSS, FOV=
(top),
(bottom).
Notes: One of the three brightest lenticulars in the Ursa
Major cluster, all of which show disturbed HI. See
Fig. 12 for a higher-resolution image of
NGC3982.
Reference: Verheijen & Zwaan, these proceedings,
p. 866.
Gzipped Postscript Version
Figure 136: The NGC1052 System.
HI: VLA D-array, 
resolution, contour
levels = 
cm
.
Optical: DSS, FOV=
(top),
(bottom).
Reference: van Gorkom, J. H., Knapp, G. R., Raimond, E.,
Faber, S. M., Gallagher, J. S. 1986, AJ, 91, 791.
Gzipped Postscript Version
Figure 137: The NGC 1023 System.
HI: VLA D-array, 
resolution,
contours=
cm.
Optical: DSS, FOV=
.
Reference: Iyer et al., these proceedings,
p. 860.
Gzipped Postscript Version
Figure 138: The NGC4111 System.
HI: VLA D-array, 45'' resolution,
contours= cm.
Optical: DSS, FOV=
(top), 
(bottom).
Notes: One of the three brightest lenticulars in the Ursa
Major cluster, all of which show disturbed HI.
Reference: Verheijen & Zwaan, these proceedings,
p. 866.
Gzipped Postscript Version
Figure 139: The NGC7426 System.
HI: VLA D-array, 
resolution,
contours= cm.
Optical: DSS, FOV=
.
Reference: Schiminovich et al., these proceedings,
p. 863.
Gzipped Postscript Version
Figure 140: The NGC 5903 System.
HI: VLA DnC-array, 
resolution,
contoured at 
cm.
Optical: DSS, FOV=
.
Notes: ESO 512-G003 does not have a known redshift.
Reference: Appleton, P. N., Pedlar, A., & Wilkinson, A. 1990,
ApJ, 357, 426.