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Table 3

Merger rate of IMCBs and breakdown into systems that merge during stable RLOF, during common envelope evolution, and during spiral-in with a white dwarf.

q-distr. β αλ AM Merger During During During spiral-in with
loss rate RLOF common envelope white dwarf

flat 1.0 1.0 L2(η = 2.3) 76% 6% 30% 65%
flat 0.5 1.0 L2(η = 2.3) 86% 23% 30% 48%
flat 0.0 1.0 L2(η = 2.3) 88% 34% 30% 37%
flat 1.0 0.5 L2(η = 2.3) 80% 6% 41% 54%
flat 0.0 0.5 L2(η = 2.3) 90% 34% 41% 26%
flat 1.0 0.1 L2(η = 2.3) 83% 6% 57% 37%
flat 0.5 0.1 L2(η = 2.3) 91% 23% 57% 20%
flat 1.0 “Dewi” L2(η = 2.3) 82% 6% 46% 49%
flat 1.0 1.0 O 74% 0% 30% 70%
flat 0.5 1.0 O 70% 0% 30% 70%
flat 1.0 1.0 L2(η = 1) 76% 3% 30% 67%
flat 0.5 1.0 L2(η = 1) 83% 7% 30% 64%
Garmany 1.0 1.0 L2(η = 2.3) 73% 4% 27% 69%
Garmany 0.0 1.0 L2(η = 2.3) 89% 38% 27% 36%
Hogeveen 1.0 1.0 L2(η = 2.3) 81% 11% 35% 54%
Hogeveen 0.0 1.0 L2(η = 2.3) 85% 26% 35% 39%

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