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Fig. 1
Distribution of the selected fields, numbered as in Table 1. The distribution is superimposed on the HI 21 cm brightness temperature map (Kalberla et al. 2005) in the radial velocity interval −100 km s-1≤ vLSR ≤ 100 km s-1. The map is in Galactic coordinates, centered on l = −60°.
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