Table 2.
Spin predictions, in Hz, for a variety of different resonance scenarios (i.e. for different azimuth number combinations; last four columns) and relative precursors timings (tp; first column) in a GRB095010-like system with a tilted binary (i.e. Θ ≠ 0°; though note that the angle does not affect the inertial-frame mode frequency).
| Relative precursor timings | (m1, m2) |
|||
|---|---|---|---|---|
| tp (s) | (1, 1) | (2, 1) | (1, 2) | (2, 2) |
| 0.5, 13 | 6.55 | 13.11 | 2.62 | 3.27 |
| 0.45, 13 | 9.54 | 19.11 | 3.82 | 4.77 |
| 0.55, 13 | 3.92 | 7.84 | 1.57 | 1.96 |
| 0.5, 12.5 | 5.41 | 10.83 | 2.16 | 2.71 |
| 0.5, 13.5 | 7.62 | 15.25 | 3.05 | 3.81 |
Notes. We use the APR4 EOS and fix the primary mass to 1.4 M⊙, assuming an equal-mass companion (q = 1).
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