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Table 3

Properties and inferred γ-ray luminosities of the pulsars and the VHE γ-ray emission regions.

Object / Region τ d P0 Ė Lγ (1)
105 yrs kpc s 10-13 s s-1 1034 erg s-1 1034 erg s-1

CXOU J164710.2–455216a 1.8 5 10.6 9.2 3 × 10-3 26
PSR J1648–4611b 1.1 5.7 0.2 0.2 21 34

HESS J1646–458 4.3 19
Region A 4.3 4.6
Region B 4.3 2.9



Obtained by scaling the observed VHE γ-ray flux between 0.1 and 100 TeV to the nominal or adopted distance of the respective object.


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