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Table 3.

56Ni mixing and hydrodynamic properties of progenitors for explosions with similar energies.

Model log (ξ/ξ0)CO Δ tRS RRS
(M) (103 km s−1) (s) (R)
B15-2 4.05 1.20 2.91 19.85 6.91 612 4.21
W16-3 6.55 1.12 2.28 13.78 4.18 873 2.73
W18 7.40 0.85 1.26 8.07 3.75 1241 3.55
W18r-2 6.65 0.76 1.10 7.85 4.14 858 2.79
W18x-2 5.13 0.93 1.89 16.56 5.85 273 1.60
W20 5.79 0.76 1.18 12.62 5.54 318 1.84
N20-P 5.98 0.91 1.38 8.39 5.19 224 2.27

Notes. The two left columns give the name of the 3D hydrodynamic explosion model and the helium-core mass of the corresponding pre-SN model. The next three columns provide the averaged characteristic velocities for the bulk of 56Ni containing 96% of the total 56Ni mass in the 3D simulations; is the weighted mean velocity of the bulk mass of 56Ni with the 56Ni mass fraction as weight function at day 150; is the maximum velocity of the bulk mass of 56Ni at the same epoch; and is the maximum velocity of the bulk mass of 56Ni at the moment just after the main shock has passed the (C+O)/He composition interface. The last three columns give the 1D hydrodynamic properties of the progenitors: (ξ/ξ0)CO is the maximum time-integrated Rayleigh–Taylor growth factor in the close vicinity of the (C+O)/He composition interface (Fig. 3); Δ tRS is the formation time of the reverse shock below the He/H composition interface, which is reckoned from the moment when the main shock crosses this composition interface; and RRS is the radius of the reverse shock at the formation epoch.

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