Table 2
Probabilities of observing a resolvable high-eccentricity DWD.
| Time (Myr) | # binaries | Expected number by cluster | Expected number by unit mass (1 /M⊙) |
|---|---|---|---|
| 11 950-12 050 | 2 | 1.3 × 10-2 | 5.6 × 10-8 |
| 11900-12 100 | 3 | 1.9 × 10-2 | 8.5 × 10-8 |
| 11 500-12 500 | 9 | 5.8 × 10-2 | 2.5 × 10-7 |
| ≥9000 Gyr | 43 | 2.3 × 10-1 | 1.2 × 10-6 |
Notes. The first column shows the snapshot in time, the second column shows the number of binaries in this snapshot from all models, the third column shows the expected number by cluster, given by the number of resolvable eccentric DWDs divided by the number of models, and the fourth column shows the expected number by unit mass, given by the number of resolvable eccentric binaries divided by the total mass of the models used.
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