Table 6
Best parameter sets of the fit of the parent particle distribution of Eq. (1) in the leptonic (subscript e for electrons) and hadronic (subscript p for protons) scenarios using solely the γ-ray data.
| Scenario | Parameter | Value | |
|---|---|---|---|
 |
[102 TeV−1 cm−2] | 7.8 ± 0.6(±3.1) | |
| Leptonic | pe | 2.33 ± 0.03(±0.33) | |
| Ecut, e | [TeV] | 27 ± 1(±12) | |
| We | [1047 erg] | 4.1 ± 0.3(±1.7) | |
 |
[104 TeV−1 cm−2] | 7.8 ± 0.3(±2.0) | |
| Hadronic | pp | 1.83 ± 0.02(±0.11) | |
| Ecut, p | [TeV] | 55 ± 6(±13) | |
 |
[1049 erg] | 7.1 ± 0.3(±1.9) | |
Notes. N0, e,p represents the differential particle number at 1 TeV, pe,p the spectral index, Ecut, e,p the cutoff energy, d the distance to the SNR (using 750 pc), n the density of the ambient medium (in cm−3), and We ,p the total energy in accelerated particles above 100 GeV for electrons in the leptonic model and above 1 GeV for protons in the hadronic model. The quoted errors represent 1σ statistical (systematic in parentheses) uncertainties.
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