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UVES interstellar observations from the Paranal Observatory Project are presented for early‐type stars located in the line of sight to the nearby open clusters IC 2391 (Omni Vel) and NGC 6475 (M7), with spectroscopic resolution R∼ 80 000 and signal‐to‐noise ratios in the Ti ii (3383 Å), Ca ii K, CH+ (4232 Å), Na i D and K i (7698 Å) lines of several hundred. The sightlines are a mixture of cluster...
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