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Table 3
He, C, N, and O abundances by number.
Star | Y He | ϵ(C) | ϵ(N) | ϵ(O) | N/C | N/O |
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MPG 355 | 0.09 | 7.39 ± 0.15 | 8.11 ± 0.16 | 8.00 ± 0.18 | 5.25 | 1.29 |
AzV177 | 0.09 | 7.17 ± 0.16 | 8.01 ± 0.22 | 7.90 ± 0.30 | 6.92 | 1.29 |
AzV 388 | 0.09 | 7.39 ± 0.15 | 7.96 ± 0.20 | 8.05 ± 0.21 | 3.71 | 0.81 |
MPG 324 | 0.09 | 7.00 ± 0.15 | 7.38 ± 0.20 | 8.00 ± 0.24 | 2.40 | 0.24 |
MPG 368 | 0.09 | 7.20 ± 0.14 | 7.70 ± 0.20 | 8.05 ± 0.18 | 3.16 | 0.45 |
MPG 113 | 0.09 | 7.52 ± 0.16 | 7.40 ± 0.34 | 8.30 ± 0.12 | 0.76 | 0.13 |
AzV 243 | 0.09 | 7.20 ± 0.20 | 7.50 ± 0.34 | 7.90 ± 0.12 | 2.00 | 0.40 |
AzV446 | 0.09 | 7.20 ± 0.22 | 7.48 ± 0.32 | 7.98 ± 0.14 | 2.04 | 0.32 |
MPG 356 | 0.09 | 7.69 ± 0.17 | 7.38 ± 0.30 | 7.98 ± 0.08 | 0.49 | 0.25 |
AzV 429 | 0.09 | 7.69 ± 0.17 | 7.08 ± 0.29 | 7.98 ± 0.22 | 0.25 | 0.13 |
MPG 523 | 0.09 | 6.38 ± 0.15 | 7.08 ± 0.35 | 7.40 ± 0.10 | 5.00 | 0.48 |
NGC 346-046 | 0.09 | 6.68 ± 0.14 | 7.56 ± 0.45 | 7.98 ± 0.37 | 7.59 | 0.38 |
NGC 346-031 | 0.09 | 7.69 ± 0.10 | 7.08 ± 0.35 | 7.98 ± 0.08 | 0.25 | 0.13 |
AzV 461 | 0.09 | 7.38 ± 0.15 | 7.38 ± 0.26 | 7.98 ± 0.35 | 1.00 | 0.25 |
MPG 299 | 0.13 | 7.69 ± 0.15 | 7.56 ± 0.44 | 8.10 ± 0.33 | 0.74 | 0.29 |
MPG 487 | 0.15 | 7.39 ± 0.20 | 6.60 ± 0.26 | 7.98 ± 0.08 | 0.16 | 0.04 |
AzV 267 | 0.09 | 7.30 ± 0.14 | 7.48 ± 0.30 | 7.98 ± 0.30 | 1.51 | 0.31 |
AzV 468 | 0.09 | 7.30 ± 0.17 | 6.30 ± 0.25 | 7.60 ± 0.14 | 0.10 | 0.05 |
AzV 148 | 0.09 | 7.69 ± 0.15 | 7.26 ± 0.30 | 7.98 ± 0.10 | 0.37 | 0.19 |
MPG 682 | 0.09 | 7.39 ± 0.14 | 6.78 ± 0.25 | 7.98 ± 0.14 | 0.25 | 0.06 |
AzV 326 | 0.09 | 7.08 ± 0.14 | 7.38 ± 0.30 | 7.98 ± 0.24 | 2.00 | 0.25 |
AzV 189 | 0.09 | 7.69 ± 0.15 | 7.38 ± 0.30 | 7.98 ± 0.21 | 0.49 | 0.25 |
MPG 012 | 0.09 | 7.34 ± 0.16 | 7.70 ± 0.21 | 8.05 ± 0.16 | 2.29 | 0.45 |
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SMC(HII) | 0.09 | 7.37 | 6.50 | 7.98 | 0.13 | 0.03 |
Notes.For comparison, we list the chemical composition determined by Kurt & Dufour (1998) for HII regions in the SMC as used in the evolutionary models by Brott et al. (2011a). By convention ϵ(X) = 12 + log [X/H].
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