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Table 3.
Spectral parameters of the LTE and blackbody model fit for the Chandra spectra.
| Teff | R(a) | log g | L |
 |
Rbb(a) | Lbb | |
|---|---|---|---|---|---|---|---|
| kK | km | 1037 erg s−1 | kK | km | 1037 erg s−1 | ||
| C0 | 561 ± 33 | 6297 ± 660 | 8.58 ± 0.11 | 3.0 ± 0.6 | 559 ± 24 | 7776 ± 984 | 4.3 ± 1.2 |
| C1 | 590 ± 25 | 5993 ± 550 | 8.63 ± 0.08 | 3.2 ± 0.7 | 589 ± 24 | 7159 ± 970 | 4.4 ± 1.4 |
| C2 | 625 ± 11 | 7351 ± 401 | 8.44 ± 0.05 | 5.9 ± 0.8 | 706 ± 18 | 6121 ± 417 | 6.7 ± 1.1 |
| C3 | 616 ± 11 | 7569 ± 432 | 8.41 ± 0.05 | 5.9 ± 0.8 | 702 ± 25 | 6191 ± 519 | 6.8 ± 1.2 |
| C4 | 623 ± 13 | 6370 ± 544 | 8.56 ± 0.07 | 4.5 ± 0.7 | 662 ± 17 | 6322 ± 533 | 5.5 ± 1.1 |
| C5 | 619 ± 12 | 6683 ± 512 | 8.52 ± 0.06 | 4.8 ± 0.7 | 675 ± 23 | 6114 ± 519 | 5.7 ± 1.1 |
Notes.
(a)
The distance to the LMC is assumed to be 50 kpc (Pietrzyński et al. 2019); NH = 5.5 × 1020 cm−2 and M = 1.1 M⊙ are fixed for all of the fits.
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