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Fig. 11


Upper panel: sky distribution of high-velocity absorbers with l > 180°, b > 30°, vLSR > 200 km s-1 and l < 180°, b < 0°, vLSR < −200 km s-1 (filled boxes) together with LG galaxies (filled circles) in the same (l,b) range. Lower panel: velocity distribution of these absorbers (colored histograms) and galaxies (gray-shaded histrograms) after transforming their velocities into the LGSR velocity frame.

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