Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae

Open Access

Fig. 17.

Same Kippenhahn plot shown in Fig. 5 for model B13.5p6.31 (Sect. 4.1) that was reran from core O-depletion without any overshooting. The zero point in the x-axis is set to the onset of convective core Si-burning. The black arrow shows the moment when core Si-burning ends.

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