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Table 3
H and Ks magnitudes, near-IR luminosities LIR, and radiation efficiencies ηIR of radio pulsars observed in the near-IR.
Pulsar name | log τ | log Ė | distance | A V | H, Ks mag | log LIR | log ηIR | Ref. |
|
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Crab | 3.1 | 38.65 | 1.73(28) | 1.62 | 14.27(5), 13.77(5) | 32.6(1), 32.9(1) | –6.1(1),–5.8(1) | (1) |
PSR 0540-69 | 3.2 | 38.17 | 5 × 104 | 0.62 | 19.33(10), 18.55(10) | 33.2(1), 33.3(1) | –5.0(1), –4.9(1) | (2) |
PSR B1509-58 | 3.2 | 37.25 | 5.2(1.4) | 4.8 | 20.6(2),19.4(1) | 31.1(2), 31.6(1) | –6.2(2),–5.7(1) | (3) |
PSR 1124-5916 | 3.5 | 37.08 | ~ 6.0 | 1.98(12) | ≥ 23.9,≥ 22.7 | ≤ 29.8, ≤ 29.9 | ≤–7.3,≤–7.2 | tw |
Vela | 4.1 | 36.84 | 0.293![]() |
0.20 | 22.04(16), 21.3(4) | 27.7(1), 28.1(2) | –9.1(1),–8.7(2) | (4) |
PSR B0656+14* | 5.0 | 34.58 | 0.288![]() |
0.09(6) | 23.22(8),22.63(13) | 27.3(1), 27.6(1) | –7.3(1),–7.0(1) | (5) |
Geminga* | 5.5 | 34.51 | 0.157![]() |
0.12(9) | 24.30(10), 23.4(4) | 26.3(1), 26.7(2) | –8.2(1),–7.7(2) | (5) |
Notes.
Reference. (1) Sollerman (2003); (2) Mignani et al. (2012); (3) Kaplan & Moon (2006); (4) Shibanov et al. (2003); (5) Koptsevich et al. (2001).
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