Fig. 5
Maximum density as a function of time for runs 3S1-hr (solid), 3S1-mr (dashed) and 3S1 (dotted). The horizontal lines correspond to the critical compression above which the Vishniac instability is triggered for supernova (lower line) and wind (thicker upper line) shells according to Vishniac & Ryu (1989). The axis on the right shows the overdensity factor over the undisturbed ambient medium.
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