Table C.3
Extinctions towards the CORNISH UCHII with visible near-IR nebulae (at least in the K band), computed from the measured near-IR fluxes using four different methods.
| Name | AH | AK | AV(H) | AV(K) | AV(J − H) | AV(H − K) |
|---|---|---|---|---|---|---|
| G010.3009−00.1477 | 4.16 | 4.03 ± 0.44 | 36.71 | 35.49 ± 3.85 | 19.60 | 9.37 |
| G010.6297−00.3380 | 1.24 | 1.9 ± 0.46 | 10.97 | 16.74 ± 4.08 | 19.74 | −1.89 |
| G010.9584+00.0221 | 3.59 | 3.89 ± 0.52 | 31.69 | 34.31 ± 4.6 | 21.31 | 3.17 |
| G011.1104−00.3985 | 3.11 | 1.36 ± 0.07 | 27.45 | 11.96 ± 0.65 | 15.63 | 32.41 |
| G011.9368−00.6158 | 4.72 | 4.29 ± 0.31 | 41.57 | 37.84 ± 2.77 | 17.57 | 13.43 |
| ... |
Notes. Aλ∕AV ratios were computed following Cardelli et al. (1989): those are ~0.28, 0.18, and 0.11, for UKIDSS λ = J, H, K, respectively, assuming RV = 3.1. All values without a quoted error are lower limits.
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