Table 1 Characteristics of glitching pulsars.
PSRτc (103 y)A〉 (10−9 d−1)G (%)Age (103 y)Ref.Embedded Image(106 K)Ref.T (108 K)
J0537−69104.932.43 ± 0.010.875 ± 0.0051–5(29, 30)1.9 ± 0.4
B0833−4511.31.96 ± 0.041.62 ± 0.035.4–16(26, 27)0.93a(28)1.2 ± 0.15
B1046−5820.41.1 ± 0.21.6 ± 0.2<1.4b(44)< 1.1
B1338−6212.11.7 ± 0.11.5 ± 0.13–30(45)1.5 ± 0.4
B1706−4417.81.1 ± 0.21.4 ± 0.35–18(46)0.5–0.8a(47)0.7 ± 0.2
B1757−2415.51.5 ± 0.21.7 ± 0.3> 10(48, 49)(50)< 1.3
B1800−2115.81.5 ± 0.21.8 ± 0.31–3b(51)Embedded Image
B1823−1321.50.8 ± 0.11.3 ± 0.2<2b(52)< 2.2
1E 1841−454.574 ± 11.2 ± 0.20.75–2.1(53)3b(28)2 ± 0.3

aFrom an atmosphere spectral model.

bFrom a blackbody spectral model.