Fig. D.1.
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Kippenhahn diagrams of the 20 M⊙ non-rotating stars from the core C-burning to the core O-burning for the three nuclear reaction rate scenarios. Dark blue shade shows the convective zones. Iso-radii contours are shown by dotted red lines. The compactness ξ is indicated by a colour bar. Top: CF88. Middle: HIN(RES). Bottom: TDHF.
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