Table 3
Spectral fit results.
| Model(1) | LMC NH | Γ | kT | R (2) | Flux(3) |
|
|
|
| [1021cm-2] | [keV] | [m] | [erg cm-2 s-1] | [erg s-1] | [%] | |||
|
|
||||||||
| XMM-Newton | ||||||||
| PL |
|
0.78 ± 0.06 | – | – | 2.07 × 10-12 | 5.5 × 1035 | – | 1.40/272 |
| PL+BBrad | 0+ 1.1 |
|
|
|
1.79 × 10-12 | 5.3 × 1035 | 53.8 | 0.98/270 |
| PL(fixed)+BBrad | 1.4 ± 0.8 | 0.7 fixed |
|
680 ± 60 | 1.78 × 10-12 | 5.3 × 1035 | 60.0 | 1.00/271 |
|
|
||||||||
| Swift (7) | ||||||||
| PL |
|
|
– | – | – | – | – | 0.90/79 |
Notes. (1) For definition of spectral models see text. (2) Radius of the emitting area. (3) Observed (0.2−10.0) keV flux derived from EPIC-pn. (4) Source intrinsic X-ray luminosity in the (0.2−10.0) keV band (corrected for absorption) for a distance to the LMC of 50 kpc (Hilditch et al. 2005). (5) Contribution of the black-body component to the total unabsorbed luminosity. (6) Degrees of freedom (d.o.f.). (7) Best-fit parameters for simultaneous fitting of the spectra from the first four Swift observations.
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