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Table A.2.

Evolutionary consequences of a 3.2 M⊙ donor star with various NS accretion efficiencies.

ε a Pi(d)b Pf(d)c MH(M⊙)d MNS(M⊙)e MsdB(M⊙)f K(kms−1)g PNS(MS)h
1.45 17.17 0.4102 × 10−3 1.8727 0.3173 91.66 0.66
1.50 16.12 0.6335 × 10−3 1.8484 0.3299 92.72 0.68
1.55 14.91 1.0380 × 10−3 1.8032 0.3468 93.65 0.74
1.60 14.81 1.9376 × 10−3 1.4745 0.3768 84.80 2.48
1.70 14.95 2.1019 × 10−3 1.4656 0.3853 84.03 2.73
0.7 3.2 1.80 15.15 2.2478 × 10−3 1.4592 0.3926 83.27 2.94
1.90 15.44 2.4361 × 10−3 1.4544 0.3989 82.43 3.13
2.00 15.77 2.5582 × 10−3 1.4508 0.4004 81.71 3.29
2.10 16.21 2.6480 × 10−3 1.4479 0.4071 80.72 3.44
2.50 18.30 2.9712 × 10−3 1.4408 0.4160 77.06 3.88
3.00 21.22 3.2089 × 10−3 1.4359 0.4221 73.05 4.26
4.00 27.27 3.4972 × 10−3 1.4313 0.4289 66.95 4.70
1.45 18.27 0.4216 × 10−3 1.7517 0.3186 87.18 0.81
1.50 17.16 0.6488 × 10−3 1.7346 0.3309 88.29 0.84
1.55 15.69 1.0592 × 10−3 1.7110 0.3475 89.93 0.88
1.60 14.86 1.9308 × 10−3 1.4707 0.3768 84.60 2.58
1.70 14.99 2.1026 × 10−3 1.4621 0.3854 83.86 2.84
0.5 3.2 1.80 15.19 2.2254 × 10−3 1.4560 0.3926 83.11 3.07
1.90 15.48 2.2539 × 10−3 1.4516 0.3984 82.30 3.26
2.00 15.81 2.4091 × 10−3 1.4480 0.4034 81.48 3.44
2.10 16.24 2.2544 × 10−3 1.4455 0.4071 80.58 3.58
2.50 18.34 2.6811 × 10−3 1.4387 0.4161 76.95 4.03
3.00 21.26 2.9630 × 10−3 1.4341 0.4222 72.98 4.43
4.00 27.31 3.4872 × 10−3 1.4289 0.4288 66.86 5.01

Notes. ε is the accretion efficiency of the NS;

(a)

initial mass of the MS star;

(b)

initial period of the systems;

(c)

final period of the systems;

(d)

total hydrogen mass;

(e)

final mass of the NS;

(f)

mass of sdBs;

(g)

RV semi-amplitude of systems;

(h)

spin period of the NS.

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