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Fig. 1.

Fig. 1. Refer to the following caption and surrounding text.

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Illustration of the different ECSN modes observed in our parameter study. Each row shows a separate simulation, with each column representing various characteristic times. In each plot, the top half indicates Ye and the bottom half ⟨A⟩ (note the varying limits in the color bars). Here, we also show contours of uniform log ρ (g cm−3). We note that in the last timestep of rho10.4_r73, we no longer fully trust the results of the simulation (e.g., the reappearance of heavier elements in the ashes is likely only an artifact) and only include this timestep as a visual indication of how the ashes get compressed into a sphere.

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