Fig. 14.

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Optical image (g-band, smoothed with a 5″-FWHM Gaussian kernel) and its contours (in white) with, overlaid, the 11″-resolution H I contour at N(H I) = 1.5 × 1020 cm−2 (in red). The black box highlights the region where the southern H I tail connects with the bump of the optical isophotes at the southern edge of the stellar body.
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