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Table 5
Predicted rates for type IIb supernovae from stable mass transfer in binaries and its dependence on different input assumptions.
Mass ratio distr. | Fav. extreme ratios | Flat | Fav. equal masses |
(x = −1) | (x = 0) | (x = 1) | |
|
|||
Fraction of binaries producing type IIb SNe via stable mass transfer | |||
0.83% | 1.33% | 1.85% | |
Number of type IIb relative to the number of all core collapse SNe | |||
(assuming that the companion does – does not produce a core collapse SNe) | |||
fbin = 25% | 0.17–0.21% | 0.27–0.33% | 0.37–0.46% |
fbin = 50% | 0.28–0.42% | 0.44–0.67% | 0.62–0.93% |
fbin = 100% | 0.42–0.83% | 0.67–1.33% | 0.93–1.85% |
Estimates of the rates assuming lower accretion efficiencies β1 | |||
β = 1.0 | 0.44–0.67% | ||
β = 0.75 | 0.60–0.92 %2 | ||
β = 0.5 | 0.69–1.06%2 | ||
β = 0.25 | 0.71–1.09%2 | ||
Assuming that all systems with orbital periods between 1000 and 2000 days produce IIb’s13 | |||
– | 2.3–3.5% | – |
Notes. See Sect. 6 for details. The rate predicted based on our standard assumptions is marked in boldface.
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