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Table 1.

Stellar parameters of the anticipated BH+O binaries obtained by V20 at BH formation, in order of increasing orbital period.

Progenitor Distance O star BH Orbital L/LEdd
system mass mass period of O star
(kpc) (M) (M) (days)
WR 155 2.99 30 12 2.6 0.161
WR 151 5.38 28 10 3.4 0.076
WR 139 1.31 28 6 5.0 0.101
WR 31 6.11 24 7 6.1 0.140
WR 42 2.44 27 14 8.7 0.156
WR 47 3.49 47 20 10.5 0.317
WR 79 1.37 24 7 10.7 0.076
WR 127 3.09 20 6 11.8 0.076
WR 21 3.99 37 10 11.8 0.341
WR 9 4.57 32 8 15.0 0.299
WR 97 2.15 30 9 18.3 0.304
WR 30 5.09 34 14 20.4 0.303
WR 113 1.80 22 8 35.9 0.054
WR 141 1.92 26 18 43.1 0.076
WR 35a 5.84 19 10 68.2 0.054
WR 11 0.34 31 8 86.8 0.107
WR 133 1.85 34 9 158.0 0.107

Notes. The BH is assumed to have formed at the end of core helium depletion of the WR star in the progenitor WR+O binaries.

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