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Table 4.

Predicted populations derived with various different assumptions.

Fiduciala Kick-265 Kick-0 Kick-BH logPq-flat SFH-S SFH-R υcrit-0.98 υcrit-0.8 NS-limit
WR+O 2.75 = = = 2.62 1.08 2.78 4.91 1.68 =
WR+Oe 3.97 = = = 5.19 1.82 4.01 1.80 5.03 =
He+OB 12.1 = = = 8.63 10.2 15.1 15.6 8.71 =
He+OBe 223 = = = 200 221 347 220 226 =
BH+OB 40.3 = = 29.5 42.1 30.5 52.3 64.0 17.1 0
BH+OBe 170 = = 96.4 226 165 261 147 194 0
NS+OB 3.74 1.41 8.02 = 2.79 = 6.75 4.39 1.84 3.74+14.2
NS+OBe 21.0 3.24 95.1 = 21.8 = 46.3 20.4 23.0 21.0+28.1
OB disr. 2.83 5.38 0 2.83+7.45 1.73 = 4.74 3.47 1.36 2.83+24.7
OBe disr. 71.5 91.0 0 71.5+74.9 93.5 = 153 70.8 73.0 71.5+138
OBe 489 = = = 546 502 811 460 521 =
− Oe 22.6 = = = 29.5 17.3 23.0 16.1 27.4 =

O stars 1072 = = = 1080 444 1083 = = =
− pre-int. 979 = = = 1010 367 = = = =
− merger 43.1 = = = 20.0 37.4 52.5 = = =
− post-int. 49.3 = = = 49.2 38.6 51.0 = = =

Notes. The predictions of fiducial model are listed for comparison purposes, and were computed with the Kroupa IMF (Eq. 7), the Sana distributions for initial mass ratios and orbital periods (Eq. 8 and Eq. 9), and with our fiducial kick velocity distributions (Table 1). A Be feature is assumed with υrot/υcrit > 0.95 and BH forms with He core mass above 6.6 M at the core He depletion. We varied these assumptions in different models (see Sect. 4 for the definitions). O stars are defined by effective temperatures above 31.6 kK, which are further divided into pre-interaction, merger products, and the MS companions in post-interaction binaries. In the table, ‘=’ means the same value as the fiducial model, and ‘+’ indicates the number change compared with the fiducial model, for example, in the NS-limit model, the number of NS+OB binaries is ‘3.74+14.2’, which means that the NS-limit predicts 14.2 more NS+OB binaries than the fiducial model.

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