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Table 3
Extinction derived from fitting the model SEDs, applying the reddening law of Moneti et al. (2001) in the infrared range.
| Object | A V | A K | Ref. |
| [mag] | [mag] | ||
|
|
|||
| WR102hb, Q 8 | 30 | 3.4 | this work (t.w.) |
| WR102ea, Q 10 | 23 | 2.6 | t.w. |
| WR102i | 24 | 2.7 | t.w. |
| WR102d | 27 | 3.0 | t.w. |
| LHO 110 | 33 | 3.7 | t.w. |
| mean | 27 ± 4 | 3.1 ± 0.5 | t.w. |
|
|
|||
| WR102c | 26 ± 1 | 2.9 ± 0.1 | Barniske et al. (2008) |
| WR102ka | 27 ± 5 | 3.0 ± 0.6 | Barniske et al. (2008) |
|
|
|||
| Quintuplet mean | 29 ± 5 | 3.28 ± 0.5 | Figer et al. (1999a) |
| Arches mean | 24.9 | 2.8 | Martins et al. (2008) |
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