Fig. 2
Maximum (top) model Ovi column densities in a 200 pc radius sphere centered at the Sun at times 0.5 through 1.0 Myr after the last SN event in the LB, overlaid by FUSE data from Savage & Lehner (2006; SL2006), Welsh & Lallement (2008; WL2008) and Barstow et al. (2010; BB2010) for observations agains white dwarfs in the up to 200 pc from the Sun. The horizontal axis indicates the integration distance for the model and the star distance from the observational data.
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