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Table 1.
Absorbed power-law model fits to Chandra spectra for three regions of G0.11−0.13 (see Fig. 3 for region definition).
| Region | NH | Γ | F2 − 10 keV | Area | χ2 (d.o.f.) |
|---|---|---|---|---|---|
| (1022 cm−2) | (erg s−1 cm−2) | (arcsec2) | |||
| “SRC” | 7.7 ± 0.6 | 1.35 ± 0.14 | 1.1 × 10−13 | 54 | 465 (478) |
| “Wings-n” | 7.6 ± 0.4 | 2.27 ± 0.12 | 1.6 × 10−13 | 420 | 506 (478) |
| “Wings-e” | 7.1 ± 0.2 | 2.40 ± 0.07 | 5.0 × 10−13 | 2213 | 645 (478) |
| Entire “IXPE” region | 8.1 ± 0.2 | 3.75 ± 0.07 | 6.4 × 10−13 | 8000 | 1010 (478) |
Notes. The observed 2−10 keV fluxes (i.e., including the effects of the low-energy photoelectric absorption) are quoted. The statistical uncertainties in the model parameters NH and Γ are given.
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