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This galaxy is at the other end of the range from NGC 4314 for many characteristics. It is hydrogen rich. It is extremely isolated (nearest companion is over one-half degree away). Star formation occurs over the entire visible disk. It has no ILR.
Similarities include a bar containing dust lanes and star formation near the nucleus.
24 August 2005
Astronomy Program · The University of Texas at Austin · Austin, Texas 78712
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