Fig. 8
FEROS and UVES spectra. Top panel: Ca ii spectra of Magellanic targets for the sightlines that have largest and smallest reduced equivalent widths between –35 and +35 km s-1. One star is from the SMC and one from the LMC although we are probing Galactic gas. Bottom panel: Corresponding data for the same two stars for Na i D. Filled lines: LHA 115-S 23 (SMC). Dotted lines: SK –67 256 (LMC).
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