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Table 6
Spectral properties of PWN G29.4+0.1 (pwn), the pulsar PS1 (psr), and HESS J1844-030 (TeV) for a distance of 6.5 kpc.
Γpwn = 1.87 | PWN photon index in the keV band |
Lpwn = 1.16 × 1034 erg s−1 | PWN luminosity in 0.5–8.0 keV |
Γpsr = 1.35 | Pulsar photon index in the keV band |
Lpsr = 6.13 × 1032 erg s−1 | Pulsar luminosity 0.5–8.0 keV |
ΓTeV = 2.48 | TeV spectral index |
LTeV = 4.61 × 1033 erg s−1 | Luminosity in 1–10 TeV |
dpsr-TeV = 1 pc | Pulsar–TeV centroid distance |
Notes. The parameters are obtained from the spectral analysis of Sects. 3.2 and 3.3, except for ΓTeV and the flux in the TeV band (used to estimate LTeV), which were taken from H.E.S.S. Collaboration (2018a).
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