Table 6
X-ray parameters for the O-type stars in N11 B.
| ID PGMW | log(LX/Lbol) (Nazé et al. 2014) | xfill | TX (MK) | rmin (R*) | log(LX/Lbol) (here) |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| 3053 | < –7.1 | 1.0 | 0.5 | 1.1 | –7.0 |
| 3058 | < –7.05 | 0.3 | 0.5 | 1.1 | –7.5 |
| 3061 | –6.57 ± 0.11 | 1.0 | 0.5 | 1.1 | –6.6 |
| 3100 | –6.86 ± 0.12 | 1.0 | 0.5 | 1.1 | –6.8 |
| 3120a | –6.53 ± 0.07 | 1.0 | 0.5 | 1.1 | –7.0 |
| 3168 | < –6.79 | 0.5 | 0.6 | 1.1 | –7.0 |
| 3204 | –6.56 ± 0.05 | 0.01 | 1.0 | 1.1 | –6.4 |
| 3223 | < –6.9 | 1.0 | 0.6 | 1.1 | –7.1 |
Notes. (1) PGMW # ID (Parker et al. 1992); (2) X-ray to bolometric luminosity ratios reported by Nazé et al. (2014); (3) fraction of electrons in the plasma phase (xfill); (4) X-ray temperature (TX); (5) minimum radius at which shock-wave occurs (rmin); (6) log(LX/Lbol) ratios needed to model UV spectral features.
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