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Table 1
Spectral fit results.
| Model1 | SMC NH | γ | kT | R2 | E WFe | Flux3 | Lx4 | χ2/d.o.f. |
| [1021 cm-2] | [eV] | [km] | [eV] | [erg cm-2 s-1] | [erg s-1] | |||
|
|
||||||||
| PL | 1.72 ± 0.25 | 0.66 ± 0.03 | – | – | – | (9.0 ± 0.3) × 10-12 | 4.0 × 1036 | 570/523 |
| PL+BB | 2.32 ± 0.44 | 0.52 ± 0.05 | 279 ± 43 | 12.2 ± 1.4 | – | (9.3 ± 0.5) × 10-12 | 4.2 × 1036 | 524/521 |
| PL+BB+Fe-line | 2.34 ± 0.45 | 0.53 ± 0.05 | 277 ± 40 | 12.2 ± 1.4 | 35 ± 30 | (9.6 ± 0.5) × 10-12 | 4.2 × 1036 | 520/520 |
| PL+DiskBB | 2.99 ± 0.54 | 0.52 ± 0.06 | 383 ± 97 | > 5.9 ± 3.5 | – | (9.3 ± 0.7) × 10-12 | 4.2 × 1036 | 528/521 |
Notes.
(2)
Radius of the emitting area (for BB) or inner disk radius (DiskBB, for the definition see text).
(4)
Source intrinsic X-ray luminosity in the 0.2–10.0 keV band (corrected for absorption) for a distance to the SMC of 60 kpc (Hilditch et al. 2005).
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