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(E-Sp)
Interacting Doubles:
2 Systems, Only 1 with HI


  figure5560
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Figure 95: The Ring Galaxy System AM 1354-250.
HI: VLA CnB+DnC-array, tex2html_wrap_inline21000 resolution, contours=tex2html_wrap_inline20100 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21006.
Reference: Higdon et al., these proceedings, p. 859.

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Figure 96: The Ring Galaxy System Arp 147.
HI: VLA B-array, tex2html_wrap_inline21008 resolution, contours=tex2html_wrap_inline20884 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21014.
Reference: Higdon et al., these proceedings, p. 859.

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Figure 97: The Lindsay-Shapley Ring.
HI: ATCA, tex2html_wrap_inline21018 resolution, contours=tex2html_wrap_inline20152 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21024.
Reference: Higdon et al., these proceedings, p. 859.

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Figure 98: The NGC 2292/3 system.
HI: VLA D-array, tex2html_wrap_inline21030 resolution, contours=tex2html_wrap_inline20046 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21036 and tex2html_wrap_inline21038.
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.

  figure5623
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Figure 99: The NGC5506/7 System.
HI: VLA C-array, tex2html_wrap_inline21042 resolution, contours=tex2html_wrap_inline20066 cmtex2html_wrap_inline20048. Optical: DSS, FOV=tex2html_wrap_inline21048.
Notes: A lower resolution map of this system showing more widely distributed gas is shown in Fig. 151.
Reference: Mundell, these proceedings, p. 411.

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Figure 100: The Arp 102 System.
HI: VLA D-array, 52'' resolution, contours=tex2html_wrap_inline21052 cmtex2html_wrap_inline20076.
Optical: DSS, FOV=tex2html_wrap_inline21056.
Reference: Higdon et al., these proceedings, p. 859.

  figure5655
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Figure 101: The Arp 104 System.
HI: VLA D-array, 52'' resolution, contours=tex2html_wrap_inline21052 cmtex2html_wrap_inline20076.
Optical: DSS, FOV=tex2html_wrap_inline21064.
Reference: Higdon et al., these proceedings, p. 859.

  figure5672
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Figure 102: The Arp 105 System.
HI: VLA C+D-array, tex2html_wrap_inline21066 resolution, contours=tex2html_wrap_inline21068 cmtex2html_wrap_inline20048.
Optical: CFHT 4m V-band, FOV=tex2html_wrap_inline21074.
Notes: In the cluster Abell 1185.
Reference: Duc, P. -A., Brinks, E., Wink, J. E., & Mirabel, I. F. 1997, A&A, 326, 537.

  figure5688
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Figure 103: The Ring Galaxy NGC2444/5.
HI: VLA C+D-array, 28'' resolution, contours=tex2html_wrap_inline20066 cmtex2html_wrap_inline20048.
Optical: KPNO 0.9m B-band, FOV=tex2html_wrap_inline21084.
Reference: Appleton, P. N., Ghigo, F. D, van Gorkom, J. H., Schombert, J. M., & Struck-Marcell, C. 1987, Nature, 330, 140.

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Figure 104: The Arp 94 System.
HI: VLA D-array, tex2html_wrap_inline21086 resolution, contours=tex2html_wrap_inline20334 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21092 (left) and tex2html_wrap_inline21094 (right).
Reference: Mundell, these proceedings, p. 411.

  figure5722
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Figure 105: The IR luminous merger Mrk 273.
HI: VLA CnB-array, tex2html_wrap_inline21096 resolution, contours=tex2html_wrap_inline20100 cmtex2html_wrap_inline20048. Optical: Lower Right: DSS, FOV=tex2html_wrap_inline20800. Other: UH 88'' R-band, FOV=tex2html_wrap_inline21108.
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.

  figure5738
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Figure 106: The Toomre Sequence merger NGC3921.
HI: VLA C+D-array, 20'' resolution, contours=tex2html_wrap_inline20178 cmtex2html_wrap_inline20048.
Optical: KPNO 2.1m R-band, FOV=tex2html_wrap_inline21118 (top), tex2html_wrap_inline20268 (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.


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Next: Interacting Doubles: Merger Remnants Up: The Gallery Previous: Interacting Doubles: No HI Tails
John Hibbard
Tue Sep 18 17:11:04 EDT 2001