Table 3
Interstellar extinction derived for the stellar sample.
| Star ID | Spec. | V (a) | B − V (a) | E(B − V) | Refs. |
|---|---|---|---|---|---|
| type | Galactic + SMC | ||||
| AV 75 | O5.5 I(f) | 12.76 | − 0.15 | 0.14 | 1, 2 |
| AV 15 | O6.5 I(f) | 13.18 | − 0.19 | 0.10 | 1, 2 |
| AV 232 | O7 Iaf | 12.31 | − 0.19 | 0.05 | 2, 4 |
| AV 83 | O7 Iaf | 13.37 | − 0.12 | 0.13 | 1 |
| AV 327 | O9.5 II-Ibw | 13.09 | − 0.16 | 0.06 | 1, 2 |
| AV 77 | O7 III | 13.95 | − 0.16 | 0.15 | 1, 2 |
| AV 95 | O7 III((f)) | 13.83 | − 0.19 | 0.04 | 1 |
| AV 69 | OC7.5 III((f)) | 13.33 | − 0.18 | 0.11 | 1, 2 |
| AV 47 | O8 III((f)) | 13.50 | − 0.18 | 0.05 | 1, 2 |
| AV 307 | O9 III | 14.02 | − 0.14 | 0.10 | 1 |
| AV 439 | O9.5 III | 14.68 | − 0.19 | 0.05 | 1, 2 |
| AV 170 | O9.7 III | 14.11 | − 0.29 | 0.06 | 1, 2 |
| AV 43 | B0.5 III | 14.08 | − 0.13 | 0.08 | 1, 3 |
Notes. (a) Photometry extracted from SIMBAD database, operated at CDS, Strasbourg, France. The colour excess, E(B − V), is divided into two contributions from the Galactic foreground and the SMC field (see above). References.The sources for the photometry are 1. Bonanos et al. (2010), 2. Cutri et al. (2003), 3. Massey (2002), and 4. Evans et al. (2006).
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