Fig. 13.
Median O VI column density NO VI (red) as a function of impact parameter b, averaged over 6800 sightlines through eight z = 0 disc galaxies simulated using the same code as the one utilized in this work. Shaded regions indicate the 1σ and 2σ deviations from the median, respectively. The observations of “star-forming” galaxies by Tumlinson et al. (2011) are shown by cyan squares.
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