Table 3
Sample stars used within this study along with spectral type, V-magnitude, interstellar extinction AV, and absolute visual magnitude MV.
Star | Cross-IDs | Spectral type | V | AV | MV |
|
|||||
N11-026 | – | O2 III(f∗) | 13.51 | 0.47 | −5.46 |
N11-031 | P3061/LH10-3061 | ON2 III(f∗) | 13.68 | 0.96 | −5.78 |
N11-038 | P3100 | O5 II(f+) | 13.81 | 0.99 | −5.68 |
Sk–66° 100 | – | O6 II(f) | 13.26 | 0.34 | −5.58 |
N11-032 | P3168 | O7 II(f) | 13.68 | 0.65 | −5.47 |
N11-045 | – | O9 III | 13.97 | 0.50 | −5.03 |
BI253 | – | O2 V((f∗)) | 13.76 | 0.71 | −5.45 |
BI237 | – | O2 V((f∗)) | 13.89 | 0.62 | −5.23 |
N11-060 | P3058/LH10-3058 | O3 V((f∗)) | 14.24 | 0.81 | −5.07 |
Sk–70° 69 | – | O5 V((f)) | 13.95 | 0.28 | −4.83 |
N11-051 | – | O5 Vn((f)) | 14.03 | 0.19 | −4.66 |
N11-058 | – | O5.5 V((f)) | 14.16 | 0.28 | −4.62 |
Sk–66° 18 | – | O6 V((f)) | 13.50 | 0.37 | −5.37 |
N11-065 | P1027 | O6.5 V((f)) | 14.40 | 0.25 | −4.35 |
N11-066 | – | O7 V((f)) | 14.40 | 0.25 | −4.35 |
N11-068 | – | O7 V((f)) | 14.55 | 0.28 | −4.23 |
N11-061 | – | O9 V | 14.24 | 0.78 | −5.04 |
N11-123 | – | O9.5 V | 15.29 | 0.16 | −3.37 |
N11-087 | P3042 | O9.5 Vn | 14.76 | 0.62 | −4.36 |
|
|||||
N11-029 | – | O9.7 Ib | 13.63 | 0.56 | −5.43 |
N11-036 | – | B0.5 Ib | 13.72 | 0.40 | −5.18 |
N11-008 | Sk–66° 15 | B0.7 Ia | 12.77 | 0.84 | −6.57 |
N11-042 | P1017 | B0 III | 13.93 | 0.22 | −4.79 |
N11-033 | P1005 | B0 IIIn | 13.68 | 0.43 | −5.25 |
N11-072 | – | B0.2 III | 14.61 | 0.09 | −3.98 |
Notes. All quantities have been taken from Mok07. Primary identifications for N11 objects are from Evans et al. (2006). Identifications starting with “Sk”, “BI”, “P”, and “LH” are from Sanduleak (1970), Brunet et al. (1975), Parker et al. (1992), and Walborn et al. (2002, 2004), respectively.
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