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Fig. 2

image

Delay-time distribution of core-collapse supernovae based on our single star models. The diagram shows the number of events per logarithmic time bin for a starburst of 106M in our standard model. The top axis shows the initial mass of single stars with the corresponding lifetime given in the bottom axis, computed with binary_c. The most massive stars evolve most rapidly and end their life after approximately 3Myr. There are no core-collapse events after approximately 48Myr when the least massive single star that can undergo core collapse explodes.

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