Table A.1.
Formation rates [10−6 yr−1] of WD+He star binaries in a MW-like galaxy of three runs and using eight selection criteria. The uncertainties are pure Poissonian statistical uncertainties.
| run | C1 | C2 | C3 | C4 |
|---|---|---|---|---|
| R1 | 426.5 ± 1.7 | 419.1 ± 1.7 | 369.5 ± 1.6 | 362.1 ± 1.6 |
| R2 | 348.6 ± 1.5 | 331.3 ± 1.5 | 305.1 ± 1.4 | 287.8 ± 1.4 |
| R3 | 579.1 ± 2.0 | 466.1 ± 1.8 | 457.0 ± 1.8 | 344.1 ± 1.5 |
| run | C5 | C6 | C7 | C8 |
| R1 | 340.4 ± 1.5 | 335.2 ± 1.5 | 293.3 ± 1.4 | 288.1 ± 1.4 |
| R2 | 249.5 ± 1.3 | 249.3 ± 1.3 | 225.1 ± 1.2 | 225.0 ± 1.2 |
| R3 | 289.2 ± 1.4 | 252.5 ± 1.3 | 211.2 ± 1.2 | 174.4 ± 1.1 |
Notes. runs:
R1: Using the same parameters as given in Table 2 of Kruckow et al. (2018) but primary and secondary masses are both taken from the range 1 to 20 M⊙.
R2: see R1 but primary and secondary masses between 1 and 10 M⊙, αRLO = 0.01, and βmin = 0.0.
R3: see R2 but αCE = 1.0 and αTH = 1.0. selection criteria:
C1: 0.4 M⊙ ≤ MHe ≤ 1.1 M⊙, MWD + MHe > 1.35 M⊙, tGW < 500 Myr.
C2: see C1 but MHe < 1.0 M⊙.
C3: see C1 but MWD + MHe > 1.4 M⊙.
C4: see C8 but tGW < 500 Myr.
C5: see C1 but tGW < 100 Myr.
C6: see C8 but MWD + MHe > 1.35 M⊙.
C7: see C8 but MHe ≤ 1.1 M⊙.
C8: 0.4 M⊙ ≤ MHe < 1.0 M⊙, MWD + MHe > 1.4 M⊙, tGW < 100 Myr.
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