Table 5.
Relative total number of events from STARTRACK that occur per simulation of 5.12 million ZAMS binaries and 5.12 million ZAMS single stars.
| Event | Rate  |
Rate rel to CCSN | |
|---|---|---|---|
| AIC | 1.9e-5 | 4e-3 | (0.36 %) |
| ECSN binary | 1.4e-4 | 3e-2 | (2.8 %) |
| ECSN single | 1.5e-5 | 2e-3 | (0.15 %) |
| Total | 1.7e-4 | 3.6e-2 | (3.31 %) |
Notes. We show birthrates of accretion-induced collapse ONe WDs to NSs (AIC), ECSNe from binaries and ECSNe from single stars. The rates are presented per total stellar mass formed in stars (rate 
) and relative to the total core collapse supernova rate from the same simulated population (percentages given in braces). A 50% binary fraction is assumed (see text).
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