Table C.1.
Number of mergers of respective types, BH–BH, BH–NS, or NS–NS, in our samples simulated for models I1 (MD17 initial binary conditions) and I2 (additionally a metallicity-dependent IMF; values given in parenthesis) for each of the 32 metallicities we computed.
Metallicity | BH–BH model I1 (I2) | BH–NS model I1 (I2) | NS–NS model I1 (I2) |
---|---|---|---|
0.0001 | 4364 (9856) | 103 (130) | 225 (42) |
0.0002 | 4924 (7982) | 61 (76) | 92 (25) |
0.0003 | 4724 (6375) | 79 (79) | 40 (13) |
0.0004 | 4480 (5387) | 112 (93) | 78 (29) |
0.0005 | 4310 (4762) | 156 (115) | 96 (20) |
0.0006 | 4184 (3988) | 132 (154) | 96 (29) |
0.0007 | 3878 (3700) | 147 (150) | 110(33) |
0.0008 | 3532 (3087) | 165 (112) | 95 (43) |
0.0009 | 3333 (2685) | 135 (81) | 110 (36) |
0.001 | 3110 (2434) | 83 (71) | 114 (35) |
0.0015 | 2002 (1339) | 199 (96) | 94 (39) |
0.002 | 1424 (809) | 194 (107) | 103 (37) |
0.0025 | 987 (474) | 206 (96) | 116 (42) |
0.003 | 931 (407) | 188 (73) | 134 (50) |
0.0035 | 1176 (530) | 214 (69) | 99 (39) |
0.004 | 1296 (1296) | 212 (212) | 49 (49) |
0.0045 | 962 (962) | 244 (244) | 66 (66) |
0.005 | 622 (622) | 232 (232) | 92 (92) |
0.0055 | 376 (376) | 275 (275) | 100 (100) |
0.006 | 288 (288) | 274 (274) | 87 (87) |
0.0065 | 202 (202) | 285 (285) | 79 (79) |
0.007 | 164 (164) | 280 (280) | 79 (79) |
0.0075 | 126 (126) | 291 (291) | 50 (50) |
0.008 | 108 (108) | 247 (247) | 47 (47) |
0.0085 | 70 (70) | 172 (172) | 57 (57) |
0.009 | 67 (67) | 148 (148) | 76 (76) |
0.0095 | 45 (45) | 112 (112) | 81 (81) |
0.01 | 40 (40) | 83 (83) | 90 (90) |
0.015 | 27 (27) | 14 (14) | 642 (642) |
0.02 | 26 (26) | 18 (18) | 535 (535) |
0.025 | 41 (41) | 18 (18) | 274 (274) |
0.03 | 55 (55) | 14 (14) | 551 (551) |
Notes. Only systems expected to merge within the Hubble time are included. We note that for metallicities Z ≥ 0.004 Z⊙, models I1 and I2 are the same, as are the simulated samples, each obtained from a population of ∼1.54 × 106 ZAMS binaries. For low metallicities Z < 0.004 Z⊙ in model I2 the number binaries at ZAMS was lower, i.e. 1 × 106.
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