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Table 3
Stellar parameters of nine Of-type stars in N 206 superbubble.
N206-FS | T ∗ | log L | log g∗ | log Ṁ | E B−V | M V | R ∗ | ν∞ | ν sin i | M ∗ 1 | log Q | log Lmec4 | Spectral type |
# | [kK] | [L⊙] | [cm s-2] | [M⊙ yr-1] | [mag] | [mag] | [R⊙] | [km s-1] | [km s-1] | [M⊙] | [s-1] | [L⊙] | |
|
|||||||||||||
66 | 35.0 | 5.22 | 4.0 | –6.38 | 0.17 | –4.61 | 11.1 | 2200 | 67 | 45 | 48.7 | 2.22 | O8 IV((f)) |
111 | 37.0 | 5.03 | 4.2 | –6.85 | 0.10 | –4.20 | 8.0 | 2500 | 43 | 37 | 48.6 | 1.86 | O7 V((f))z |
131a2 | 36.0 | 5.80 | 3.6 | –5.50 | 0.11 | –6.23 | 20.5 | 1500 | 96 | 61 | 49.4 | 2.77 | O6.5 II(f) |
131b3 | 30.0 | 5.04 | 3.8 | –6.57 | 0.12 | –5.00 | 12.3 | 1900 | 79 | 35 | 48.0 | 1.91 | O9.7 IV |
162 | 34.0 | 5.60 | 3.8 | –6.03 | 0.20 | –5.67 | 18.2 | 2100 | 83 | 77 | 49.1 | 2.53 | O8 IV((f))e |
178 | 35.0 | 5.22 | 4.0 | –6.38 | 0.14 | –4.55 | 11.1 | 2200 | 79 | 45 | 48.7 | 2.22 | O7.5 III((f)) |
180a2 | 50.0 | 6.11 | 4.2 | –5.32 | 0.16 | –5.77 | 15.2 | 28007 | 128 | 133 | 50.0 | 3.49 | O2 V((f*)) |
180b3 | 32.0 | 4.91 | 4.2 | –6.62 | 0.18 | –4.50 | 9.3 | 2900 | 42 | 50 | 48.0 | 2.21 | O8 IV |
1875 | 38.0 | 6.28 | 3.6 | –4.80 | 0.19 | –6.70 | 31.9 | 23007 | 116 | 148 | 50.0 | 3.86 | O4 If |
193 | 36.0 | 5.20 | 4.2 | –6.36 | 0.20 | –4.44 | 10.3 | 2900 | 103 | 61 | 48.7 | 2.48 | O7 V((f))z |
2146 | 38.0 | 6.10 | 3.6 | –4.93 | 0.33 | –6.26 | 26.0 | 23007 | 98 | 98 | 49.8 | 3.71 | O4 If |
Notes.
(5)
When strong clumping (D = 20 and RD = 0.05 R∗) is adopted then log Ṁ = −5.59 M⊙ yr-1 and log Lmec = 3.05 L⊙. The X-ray field is included in this model, with X-ray luminosity LX = 4.7 × 1033 erg s-1.
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