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Fig. 19


H i contours of WVFSCC 125550+041348 at levels of 1, 2, 4 and 8 Jy km s-1 overlaid on a red band, second generation DSS images. The main galaxy NGC 4808 has a long tail of H i towards the south, connecting two other galaxies. South-East of the main galaxy is a very faint signal possibly associated with another galaxy.

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