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Table 2
Pulsars with small characteristic ages in globular clusters.
| NGC: PSR | P | Ṗ | B | τ c | ||
| (s) | (10-15) | (1012 G) | (1010 yr) | |||
|
|
||||||
| 1 | 6342: B1718−19 | 1.0040 | 1.59000 | 1.263 | 0.001 | |
| 2 | 6624: B1820−30B | 0.3786 | 0.03150 | 0.109 | 0.019 | |
| 3 | 6624: J1823−3021C | 0.4059 | 0.22400 | 0.302 | 0.003 | |
| 4 | 6440: B1745−20 | 0.2886 | 0.39933 | 0.339 | 0.001 | |
| 5 | 7078: B2127+11C | 0.0305 | 0.00499 | 0.012 | 0.010 | |
| 6 | 6624: B1820−30A | 0.0054 | 0.00338 | 0.004 | 0.003 | |
| 7 | 6626: B1821−24A | 0.0031 | 0.00155 | 0.002 | 0.003 | |
Notes. Because the age of the GCs in our galaxy is close to 1010 yr, the last column may also be read as giving the characteristic age as fraction of the cluster age. References for these pulsars are given in Sect. 3.2.
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