Fig. 6.
Cumulative distributions of the time of the strongest encounter (orange) and the moment of the first preserving supernova (blue) for the systems equivalent to the solar-system. We only plot the distributions for the first 9 supernovae from the 180 simulations with N = 2500 and rvir = 0.75 pc. A similar distribution of supernova distance was also presented in Parker et al. (2014).
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