Fig. 5.
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ξ2.5 vs. initial 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 represented in red, green and black, respectively. The squares mark the occurrence of CHE. The left and middle blue triangles indicate model calculations from Li et al. (2023) (Z = 0.0017), and the right blue triangle denotes the rapidly rotating model from Aguilera-Dena et al. (2020) (1/50 Z⊙). The dashed lines mark explosion criteria for ξ2.5: the black line shows O’Connor & Ott (2011), and others from our results.
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