Summary of the binary properties for each case examined. We report the masses m1 and m2 of each star in the binary, the mass ratio q = m2/m1, and the time after merger.
| Case . | m1(M⊙) . | m2(M⊙) . | q . | Time after merger (ms) . |
|---|---|---|---|---|
| 1 | 1.4 | 1.4 | 1.00 | ≈38 |
| 2 | 1.3 | 1.3 | 1.00 | ≈18 |
| 3 | 1.3 | 1.2 | 0.92 | ≈18 |
| Case . | m1(M⊙) . | m2(M⊙) . | q . | Time after merger (ms) . |
|---|---|---|---|---|
| 1 | 1.4 | 1.4 | 1.00 | ≈38 |
| 2 | 1.3 | 1.3 | 1.00 | ≈18 |
| 3 | 1.3 | 1.2 | 0.92 | ≈18 |
Summary of the binary properties for each case examined. We report the masses m1 and m2 of each star in the binary, the mass ratio q = m2/m1, and the time after merger.
| Case . | m1(M⊙) . | m2(M⊙) . | q . | Time after merger (ms) . |
|---|---|---|---|---|
| 1 | 1.4 | 1.4 | 1.00 | ≈38 |
| 2 | 1.3 | 1.3 | 1.00 | ≈18 |
| 3 | 1.3 | 1.2 | 0.92 | ≈18 |
| Case . | m1(M⊙) . | m2(M⊙) . | q . | Time after merger (ms) . |
|---|---|---|---|---|
| 1 | 1.4 | 1.4 | 1.00 | ≈38 |
| 2 | 1.3 | 1.3 | 1.00 | ≈18 |
| 3 | 1.3 | 1.2 | 0.92 | ≈18 |
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