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Table 7

Thermal emission properties.

Pulsar name τ RPC Bd d kT RBB Lbol Ref.
Myr m 1012 G kpc keV m erg s−1
B0114+58 0.28 455 0.8 1.77 ± 0.53b 0.17 ± 0.02 (1)
J0633+1746 0.34 297 1.6 0.16 ± 0.03 64 ± 16 (2)
B0656+14 0.11 233 4.7 0.28 ± 0.03a 0.108 ± 0.003 1813 ± 151 (1.4 ± 0.4) × 1031 (2)
B0943+10 4.98 138 2.0 0.89 ± 0.27b 0.245 ± 0.025 (3)
B1055−52 0.54 326 1.1 0.35 ± 0.15c 0.154 ± 0.005 215 ± 28 (2)
J1740+1000 0.11 369 2.7 1.23 ± 0.37b (4)
                 
B1822−09 0.23 165 6.4 (5)
                 
B1929+10 3.10 304 0.5 (6)
                 
B0355+54 0.56 366 0.8 ~0.16 ~250 (7)
B0628−28 2.77 130 3.0 (1)
                 
B0834+06 2.97 128 3.0 0.19 ± 0.06b (8)

Notes. (a) Parallax measurements (Verbiest et al. 2012). (b)Inferred from the dispersion measure (Yao et al. 2017). Assumed error 30%. (c) Mignani et al. (2010). References: (1) this paper; (2) De Luca et al. (2005); (3) Mereghetti et al. (2016); (4) Kargaltsev et al. (2012); (5) Hermsen et al. (2017); (6) Misanovic et al. (2008); (7) Klingler et al. (2016); (8) Gil et al. (2008).

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