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Table 4

Results for the X-ray spectral fitting of the knots.

Component Γa NHb Kc reduced χ2 d.o.f.
(× 1020 cm−2) (× 10−5 photons keV−1 s−1) (× 10−13 erg cm−2 s−1)
       
HST-1 H1 2.25 ± 0.05 4.74 94.88 44.73 ± 0.62 0.98 2174
             
HST-1 H5 2.31 ± 0.06 1.21 50.59 23.62 ± 0.59 0.93 1293
             
HST-1 L 2.27 <1.21 14.53 6.86 ± 0.15 1.08 1801
             
D 2.22 ± 0.03 2.50 ± 0.5 17.11 ± 0.4 8.13 ± 0.10 0.72 5526
             
E 2.35 ± 0.05 2.34 4.10 1.91 ± 0.04 0.70 2726
             
F 2.61 <0.46 2.15 1.00 ± 0.01 0.74 1720
             
I 2.50 <0.57 1.20 0.56 ± 0.04 1.02 576
             
A 2.41 ± 0.02 <0.10 21.22 9.85 ± 0.02 0.90 4811
             
B 2.35 <0.8 3.49 1.63 ± 0.02 0.89 2480
             
C 1.89 <0.85 1.78 0.94 ± 0.02 0.64 2145
             

F 2.79 ± 0.04 2.4 (frozen) 2.36 ± 0.05 1.13 ± 0.02 0.75 1721
             
I 2.60 ± 0.04 2.4 (frozen) 1.28 ± 0.03 0.60 ± 0.01 1.04 577
             
A 2.55 ± 0.01 2.4 (frozen) 23.10 ± 0.2 10.74 ± 0.05 0.96 4812
             
B 2.49 ± 0.03 2.4 (frozen) 3.85 ± 0.06 1.79 ± 0.02 0.90 2481
             
C 2.01 ± 0.04 2.4 (frozen) 1.99 ± 0.05 1.0 ± 0.02 0.65 2146
             

Notes. All errors are at a 90% confidence level. H1, H5, and L are defined as shown in Fig. 3. (a) Photon index. (b) Equivalent hydrogen-absorbing column density. (c) Amplitude of power-law model. (d) Total integrated energy flux over 0.3–7 keV. The bottom part provides the results if NH is frozen to the Galactic value.

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