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Table 2

Summary of selected systems which evolved successfully to AIC and later produced recycled pulsars.

Model t RLO X c ΔtCV Kick∗ Angles v sys Δtdetach ΔtLMXB M WD M NS ΔMNS P spin t total
M ⊙ days Myr Myr M ⊙ days km s-1 deg km s-1 Myr days Myr M ⊙ days M ⊙ M ⊙ ms Myr
MS1W 3.00 1.50 294 0.12 1.27 1.65 0.78 0 12 0.054 0.88 335 0.310 17.8 1.46 0.18 1.2 630
MS2W 2.80 5.00 1250 0.00 0.51 1.56 3.19 0 8 0.064 3.65 4 0.411∗∗ 37.2 1.31 0.03 4.7 1250
MS3 2.60 1.00 357 0.29 1.90 1.99 0.68 0 13 0.003 0.76 1240 0.262 23.8 1.55 0.27 0.9 1600
MS4 50 (0, 0) 7 0.097 1.12 891 0.273 31.8 1.61 0.33 0.8 1250
MS5 450 (107, 90) 180 165 1.83 214 0.298 43.6 1.66 0.38 0.7 736
MS6 2.50 1.00 403 0.28 1.98 1.99 0.72 0 13 0.003 0.80 1180 0.264 24.8 1.56 0.28 0.9 1590
MS7 2.50 1.50 504 0.08 1.68 1.97 1.07 0 11 0.010 1.20 252 0.301 26.4 1.56 0.28 0.9 758
MS8 50 (0, 0) 9 0.19 1.87 159 0.307 41.0 1.64 0.36 0.7 665
MS9 450 (116, 90) 183 58 2.88 30 0.320 52.7 1.44 0.16 1.3 594
MS10 2.50 2.50 539 0.00 0.67 1.88 1.76 0 9 0.048 1.99 12 0.335∗∗ 33.4 1.35 0.07 2.5 552
MS11 2.50 3.00 545 0.00 0.63 1.92 2.12 0 9 0.124 2.39 11 0.341∗∗ 38.3 1.34 0.06 2.8 557
MS12 2.20 1.00 584 0.26 2.08 1.85 0.79 0 12 0.016 0.89 986 0.269 27.3 1.60 0.32 0.8 1570
MS13 50 (0, 0) 8 100 1.34 450 0.285 37.4 1.67 0.39 0.7 1140
MS14 450 (112, 90) 189 264 2.02 108 0.297 47.3 1.58 0.30 0.8 958
MS15 2.20 2.00 765 0.00 1.05 1.84 1.58 0 10 0.046 1.79 29 0.295 40.1 1.42 0.14 1.5 795
MS16 2.20 2.50 770 0.00 0.91 1.88 1.98 0 9 0.178 2.24 25 0.303 48.1 1.40 0.12 1.7 796
MS17 2.00 1.00 788 0.24 4.92 1.59 0.84 0 12 0.487 0.96 839 0.272 28.3 1.59 0.31 0.8 1630
MS18 2.00 2.00 1010 0.00 2.02 1.63 1.68 0 9 6.74 1.92 66 0.297 41.8 1.44 0.16 1.3 1090
MZ1 2.00 1.00 594 0.00 1.00 1.30 0.99 0 11 0.003 1.16 22.5 0.310 20.5 1.36 0.08 2.3 618
MZ2 1.80 4.00 811 0.00 1.95 1.44 3.62 0 7 1.62 4.17 56 0.345 58.6 1.44 0.16 1.3 871
MZ3 50 (0, 0) 16 15.0 8.19 47 0.367 95.3 1.44 0.16 1.3 875
MZ4 450 (161, 90) 218 21.4 10.57 41 0.377 114.7 1.44 0.16 1.3 875
MZ5 1.40 1.00 1750 0.00 4.52 0.957 1.26 0 9 0.228 1.51 165 0.285 21.7 1.45 0.17 1.3 1920
GS1 1.10 80 8510 0.00 2.29 0.711 134 0 2 3.83 163 5.01 0.408 552 1.31 0.02 6.4 8520
GS2 1.10 180 8520 0.00 1.69 0.685 325 0 1 1.91 394 2.40 ~0.47∗ ∗ ∗ >919 1.29 0.011 14 8530
GS3 1.00 400 13600 0.00 1.98 0.577 907 0 1 2.51 1110 ~0.01 ~0.50∗ ∗ ∗ ~1400 1.280 0.000 500 13600
GS4 0.90 160 19100 0.00 3.63 0.529 372 0 1 0.80 459 CE ~0.46∗ ∗ CE 1.280 0.000 – –
GSZ1 1.00 250 6330 0.00 2.02 0.622 481 0 1 0.30 587 2.32 ~0.53∗ ∗ ∗ >819 1.32 0.010 11.0 6340
He1 1.40 0.04 0.014 0.97∗ 2.77 1.05 0.039 0 30 3.59 0.046 7.96 0.670∗∗ 0.072 1.32 0.04 3.8 14.3
He2 1.40 0.05 2.49 0.51∗ 5.87 1.03 0.044 0 29 0.073 0.051 1.32 0.719∗∗ 0.097 1.294 0.014 8.4 9.75
He3 1.40 0.10 7.12 0.00∗ 0.20 1.12 0.100 0 23 0.043 0.118 0.392 0.821∗∗ 0.199 1.284 0.004 21 7.75
He4 1.20 0.05 4.26 0.00∗ 5.60 0.797 0.054 0 25 0.256 0.066 1.07 0.703∗∗ 0.082 1.291 0.011 10 11.2
He5 1.20 0.60 21.9 0.00∗ 0.11 0.921 0.707 0 11 0.005 0.84 0.121 0.833∗∗ 1.03 1.281 0.001 60 22.1
He6 50 (0, 0) 18 0.017 1.30 0.113 0.836∗∗ 1.53 1.281 0.001 60 22.1
He7 450 (120, 90) 267 0.023 1.66 0.108 0.838∗∗ 1.95 1.281 0.001 60 22.1
He8 1.10 1.20 32.4 0.00∗ 0.16 0.829 1.52 0 8 0.012 1.81 0.032 0.826∗∗ 1.82 1.280 0.000 200 32.6

Notes. See first paragraph of Sect. 4 for explanations of all the variables (∗ =Yc, ∗ ∗ = (hybrid) CO WD, ∗ ∗ ∗ = CO WD after He-flash on the RGB, CE = onset of a common envelope).

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