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Table 2
Some characteristics of the double neutron star systems with their approximate orbital parameters.
| Pulsar | P | Ė | d | Ωp | χ | i | δ |
|
Reference |
| (ms) | (1026W) | (kpc) | (deg/yr) |  /kpc2) |
|||||
|
|
|||||||||
| J0737-3039A | 22.7 | 5.9 | 1.1 | 4.8 | 90 | 90 | ≲ 6 | 2.0 | Ferdman et al. (2013) |
| J0737-3039B | 2773 | 0.0017 | 1.1 | 5.1 | 70 | 90 | 138 | 0.03 | Perera et al. (2010) |
| J1906+0746 | 144 | 270 | 4.5 | 2.2 | 81 | 42-51 | 89 | 0.81 | Desvignes et al. (2013) |
| B1913+16 | 59 | 1.7 | 7.1 | 1.2 | 47 | 157 | 21 | 0.026 | Weisberg & Taylor (2002) |
| B1534+12 | 37.9 | 1.8 | 1.0 | 0.5 | 110 | 78 | 30,100? | 1.3 | Konacki et al. (2003) |
| J1141-6545 | 394 | 2.8 | 3.0 | 1.4 | 160 | 73 | 93 | 0.19 | Manchester et al. (2010) |
Notes. Angles are given in degrees according to the fits given in the corresponding references. We also computed the figure-of-merit as defined by Abdo et al. (2013). Distance are from the ATNF catalogue.
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