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Table 3

Hemispheric ejecta yields of helium and metals, and total nickel mass for the high-kick models W15-1 and W15-2, and the moderate-kick models L15-1 and L15-2.

Model 4He  [M⊙]  12C  [10-1 M⊙]  16O  [10-1 M⊙]  20Ne  [10-2 M⊙]  24Mg  [10-2 M⊙] 
North South North South North South North South North South
W15-1 2.78 2.66 1.18 1.10 3.68 3.75 8.90 8.49 2.41 2.85
W15-2 2.78 2.65 1.16 1.12 3.43 3.84 8.67 8.49 2.16 2.86
L15-1 2.39 2.34 0.90 0.87 2.77 2.89 5.00 5.06 2.12 2.49
L15-2 2.40 2.39 0.89 0.87 2.85 2.79 5.21 4.88 2.47 2.42
Model 28Si  [10-2 M⊙]  40Ca  [10-2 M⊙]  44Ti  [10-3 M⊙]  56Ni  [10-2 M⊙]  Tracer  [10-2 M⊙]  Total 56Ni Mass  [M⊙] 
North South North South North South North South North South
W15-1 1.88 2.92 1.33 4.81 0.68 2.43 1.26 4.28 2.23 6.08 0.055–0.139
W15-2 1.74 2.83 1.27 4.66 0.81 2.17 1.37 4.09 2.22 6.27 0.055–0.139
L15-1 1.75 2.33 1.76 2.47 1.49 2.40 1.34 1.87 4.78 7.20 0.032–0.152
L15-2 2.13 2.15 2.54 2.74 2.32 2.55 1.81 1.89 8.68 9.74 0.037–0.221

Notes. The numbers are integral values of the elemental abundances in the whole stellar matter that gets expelled by the supernova explosion. The tracer column provides the yield of Fe-group nuclei in neutrino-processed ejected material, some undetermined fraction of which may be 56Ni. The north-polar direction is defined to coincide with the NS kick direction.

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