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Table 6

Calculated luminosity at different wave bands and synchrotron cooling break energies in the sample.

PWN L R L X L γ L bol E s L s
(1.4 GHz) (1–10 keV) (1–10 TeV) MeV
erg/s erg/s erg/s erg/s erg/s

Young PWNe

N158A
G21.5-0.9
Crab nebula
Kes 75
G310.6-1.6
3C 58

Evolved PWNe

HESS J1813-178
G54.1+0.3
G292.0+1.8
G0.9+0.1
MSH 15-52
N157B

Mature/old PWNe

HESS J1356-645
CTA 1
HESS J1418-609
HESS J1420-607
HESS J1119-614
HESS J1303-631 4.17 × 10-3

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