Extended Data Table 4 Example calculations of supernova nucleosynthesis models
From: Solar abundance ratios of the iron-peak elements in the Perseus cluster
- The first three columns indicate the name and combination of supernova models and the fourth column presents the assumed index of the IMF. fCC = NCC/(NIa + NCC),
and fFe,Ia are the number fraction of core-collapse supernovae, the number fraction of near-MCh type Ia supernovae and the mass fraction of Fe originating from type Ia supernovae, respectively. The remaining columns indicate abundance ratios relative to the solar values25. SN, supernova; HN, hypernova.
and fFe,Ia are the number fraction of core-collapse supernovae, the number fraction of near-MCh type Ia supernovae and the mass fraction of Fe originating from type Ia supernovae, respectively. The remaining columns indicate abundance ratios relative to the solar values