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Galaxies with One-Sided HI Extensions


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Figure 18: The NGC 3885 System.
HI: VLA D-array, 60'' resolution, contours=tex2html_wrap_inline20066 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20202.
Notes: The companion galaxy has no cataloged counterpart.
Reference: Hameed & Young, these proceedings, p. 857.

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Figure 19: The UGC 8331 System.
HI: WSRT, 30'' resolution, contours=tex2html_wrap_inline20100 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20210.
Reference: 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.

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Figure 20: The UGC11152 System.
HI: VLA D-array, 66'' resolution, contours=tex2html_wrap_inline20178 cmtex2html_wrap_inline20048.
Optical: WIYN B-band, FOV=tex2html_wrap_inline20220.
Reference: Pisano & Wilcots, these proceedings, p. 501.

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Figure 21: The NGC4639/4654 System.
HI: VLA C+D-array, tex2html_wrap_inline20222 resolution, contours=tex2html_wrap_inline20066 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20228.
Reference: Phookun, B., & Mundy, L. G. 1995, ApJ, 453, 154.

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Figure 22: The ``Superthin'' galaxy ESO 572-G045.
HI: VLA C+D-array. Left panel: 40'' resolution, contours=tex2html_wrap_inline20100 cmtex2html_wrap_inline20238. Middle panel: tex2html_wrap_inline20240 resolution, contours=tex2html_wrap_inline20100 cmtex2html_wrap_inline20238. Right panel: tex2html_wrap_inline20246 resolution, contours=tex2html_wrap_inline20248 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20252.
Notes: Companion to the merging system NGC4038/9 (see Fig. 65).
Reference: Hibbard, J.E., van der Hulst, J. M., Barnes, J. E., & Rich, R. M. 2001, AJ, in press.

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Figure 23: The IC 3355 System.
HI: VLA D-array, tex2html_wrap_inline20254 resolution, contours=tex2html_wrap_inline20188 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20260.
Notes: Member of the Virgo cluster near M86. See also Fig. 167.
Reference: Observed in the field of NGC 4406 (M86) by Li & van Gorkom, these proceedings, p. 637.

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Figure 24: The NGC4522 System.
HI: VLA C-array, tex2html_wrap_inline20262 resolution, contours=tex2html_wrap_inline20100 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20268.
Reference: Kenney, van Gorkom, & Vollmer, these proceedings, p. 861.

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Figure 25: The Arp 120 System.
HI: VLA D-array, tex2html_wrap_inline20254 resolution, contours=tex2html_wrap_inline20188 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20276.
Notes: Member of the Virgo cluster near M86. See also Fig. 167.
Reference: Observed in the field of NGC 4406 (M86) by Li & van Gorkom, these proceedings, p. 637.

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Figure 26: The NGC3079 System.
HI: VLA D-array, contours=(0.5, 1, 1.5, 2.4, 4, 10, 15, 25, 45)tex2html_wrap_inline20278 cmtex2html_wrap_inline20076. Resolution: tex2html_wrap_inline20282 NGC 3079; tex2html_wrap_inline20284 others.
Optical: DSS, FOV=tex2html_wrap_inline20286.
Reference: Irwin, J.A., Seaquist, E.R., Taylor, A.R., & Duric, N. 1987, ApJ, 313, L91.


next up previous
Next: Detached HI Clouds Up: The Gallery Previous: Two-Sided Warps
John Hibbard
Tue Sep 18 17:11:04 EDT 2001