Fig. 4

Model for the ISM clouds present in the LS III +46 11 and LS III +46 12 sightlines. Cloud σ1 is of low density, not associated with the cluster, and affects both sightlines similarly. Cloud σ2 is also of low density, is the skin of the cloud associated with the cluster, and is longer along the LS III +46 12 sightline. Cloud ζ is of high density, is the core of the cloud associated with the cluster, and affects LS III +46 11 exclusively (or, at least, to a much larger degree than LS III +46 12).
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