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Table 2
Numerical values used to evaluate the hypothesis of a quasi-periodicity induced by the precession of the periastron of PSR 1931+24.
| Name | Notation | Value |
|
|
||
| Rotation period of the periapsis | P per | 70 days |
| Orbital period | P orb | 7.8 min |
| Semi-major axis | a | 105 km = 2.5Rlc |
| Eccentricity | e | 0 < e < 0.65 |
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