Fig. 6.
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ξ2.5 vs. CO-core mass for models with varying initial rotational velocities Vini and metallicities. The left, middle, and right panels correspond to models with Vini = 0, 300 km s−1, and 600 km s−1, respectively. Metallicities of Z⊙, 1/10 Z⊙, and 1/50 Z⊙ are shon in red, green, and black, respectively. The squares mark the occurrence of CHE.
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