Fig. 12

Isosurfaces of the distributions of unshocked Fe (red) and Ti (blue) at the age of Cas A for different values of the mass fractions (decreasing from left to right; see the values reported at the end of the caption) and different viewing angles (front and side views) for models W15-2-cw-IIb-HD and W15-2-cw-IIb-HD+dec. The values of the mass fractions are selected so that the corresponding isosurfaces enclose, from left to right, 30, 50, 75, and 95% of the total mass of the respective unshocked species. The red isosurfaces correspond to a value of Fe density in model W15-2-cw-IIb-HD (W15-2-cw-IIb-HD+dec) which is, in units of 10−26 g cm−3, 119 (89), 95 (81), 71 (70), 40 (55), respectively; the blue isosurfaces correspond to a value ofTi density in model W15-2-cw-IIb-HD (W15-2-cw-IIb-HD+dec) which is, in units of 10−27 g cm−3 (considering the tracer-particle-based post-processing with a large nuclear network, Wongwathanarat et al. 2017, but not considering its decay in 44Ca), 2.1 (1.7), 1.7 (1.4), 1.2 (1.1), 0.7 (0.8), respectively (considering the decay of 44Ti in 44Ca, these values are scaled by a factor of 0.027, for an e-folding time of 90 yr). See online Movie 3 for an animation of these data; a navigable 3D graphic of these distributions is available at https://skfb.ly/6UMxI.
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