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Fig. 8


Sky distribution of sightlines in our COS sample in an Hammer-Aitoff projection of Galactic coordinates overlaid on a map of 21 cm emission for | vLSR | ≤ 500 km s-1 based on the LAB survey (Kalberla et al. 2005; courtesy Tobias Westmeier). The color scheme is similar to that in Fig. 2.

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