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Convective core overshooting influences stars' internal structure, determining which ones become black holes. It also affects BH masses and the pre-supernova location of stars in the HRD.💫
Increased overshooting results in initially lower-mass stars forming black holes.
Duresa temaj@DuresaTemaj
My first author paper on Convective core-overshooting on the final fate of massive stars is accepted for publication in A&A: arxiv.org/abs/2311.05701 We found that black hole progenitors have specific luminosity and CO core masses at the end of core carbon burning.
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