Table 4.
Results of the spectral modeling.
| Parameter | Model/Unit | Disk | Halo | East | West |
|---|---|---|---|---|---|
| cstat/d.o.f. | APEC only | 1.12 | 1.10 | 1.09 | |
| kT | keV | ![]() |
![]() |
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|
| Z/Z⊙ | 0.1 | 0.1 | 0.1 | ||
| normapec | cm−5 | ![]() |
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|
| cstat/dof | APEC+POWERLAW | 1.00 | 1.11 | 1.10 | 1.09 |
| kT | keV | ![]() |
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| Z/Z⊙ | 1.0 | 0.1 | 0.1 | 0.1 | |
| normapec | cm−5 | ![]() |
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| Γ | ![]() |
1.7 | 1.7 | 1.7 | |
| normPL | cts keV−1 cm−2 s−1 | ![]() |
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Notes. Fit results for the disk, the halo out to r = 5 ′, and the two regions of enhanced emission. The top section of the table displays the results for the APEC only model; the lower section displays the results for the APEC+POWERLAW model. The metal abundance Z and the power-law indices of the halo regions were fixed to the presented values.
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