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(EpecH)
Normal Early Types with Peculiar HI


  
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Figure 130: The Polar Ring Galaxy UGC 7576.
HI: VLA C-array, 10'' resolution.
Optical: Top: DSS. Bottom: WIYN V-band image, FOV=tex2html_wrap_inline21330.
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.

  figure6186
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Figure 131: The IC2006 System.
HI: VLA D-array, 40'' resolution, contours=tex2html_wrap_inline20334 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21340.
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.

  figure6198
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Figure 132: The NGC 2810 System.
HI: VLA D-array, tex2html_wrap_inline21342 resolution, contours=tex2html_wrap_inline20188 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21348 (top), tex2html_wrap_inline21350 (bottom).
Reference: Schiminovich et al., these proceedings, p. 863.

  figure6214
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Figure 133: The NGC 2768 System.
HI: VLA D-array, tex2html_wrap_inline21352 resolution, contours=tex2html_wrap_inline20188 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21358.
Reference: Schiminovich et al., these proceedings, p. 863.

  figure6229
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Figure 134: The NGC4026 System.
HI: VLA D-array, 45'' resolution, contours=tex2html_wrap_inline20188 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21366.
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.

  figure6247
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Figure 135: The NGC 3998 System.
HI: VLA D-array, 45'' resolution, contours=tex2html_wrap_inline20188 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline20202 (top), tex2html_wrap_inline21376 (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.

  figure6270
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Figure 136: The NGC1052 System.
HI: VLA D-array, tex2html_wrap_inline21378 resolution, contour levels = tex2html_wrap_inline21380 cmtex2html_wrap_inline20076.
Optical: DSS, FOV=tex2html_wrap_inline21384 (top), tex2html_wrap_inline21386 (bottom).
Reference: van Gorkom, J. H., Knapp, G. R., Raimond, E., Faber, S. M., Gallagher, J. S. 1986, AJ, 91, 791.

  figure6284
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Figure 137: The NGC 1023 System.
HI: VLA D-array, tex2html_wrap_inline21388 resolution, contours=tex2html_wrap_inline20136 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21394.
Reference: Iyer et al., these proceedings, p. 860.

  figure6298
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Figure 138: The NGC4111 System.
HI: VLA D-array, 45'' resolution, contours=tex2html_wrap_inline20188 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21402 (top), tex2html_wrap_inline21404 (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.

  figure6320
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Figure 139: The NGC7426 System.
HI: VLA D-array, tex2html_wrap_inline21406 resolution, contours=tex2html_wrap_inline20334 cmtex2html_wrap_inline20048.
Optical: DSS, FOV=tex2html_wrap_inline21412.
Reference: Schiminovich et al., these proceedings, p. 863.

  figure6341
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Figure 140: The NGC 5903 System.
HI: VLA DnC-array, tex2html_wrap_inline21416 resolution, contoured at tex2html_wrap_inline21418 cmtex2html_wrap_inline20076.
Optical: DSS, FOV=tex2html_wrap_inline21422.
Notes: ESO 512-G003 does not have a known redshift.
Reference: Appleton, P. N., Pedlar, A., & Wilkinson, A. 1990, ApJ, 357, 426.


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Next: Intergalactic HI Debris Up: The Gallery Previous: Pec Es with HI Within Body
John Hibbard
Tue Sep 18 17:11:04 EDT 2001