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Table A.1
Properties of the sources and results of the SED fit procedure for the far outer Galaxy sample.
| Source | l | b | Dist.a | RGC a | Diam. | Td | Lbol | Mdust | Σdust b |
| deg | deg | [kpc] | [kpc] | [″] | [K] | [10xL⊙] | [10xM⊙] | [10x g cm-2] | |
|
|
|||||||||
| WB89_898 | 217.604 | −2.617 | 8.8 | 16.4 | 109 | 24.1 ± 5.7 | 3.65 ± 0.24 | 0.15 ± 0.19 | −3.84 ± 0.19 |
| WB89_986 | 229.772 | 0.060 | 7.9 | 14.9 | 120 | 22.0 ± 4.7 | 3.48 ± 0.28 | 0.35 ± 0.18 | −4.04 ± 0.18 |
| WB89_909 | 217.331 | −1.369 | 6.3 | 14.0 | 120 | 20.6 ± 2.6 | 3.72 ± 0.20 | 0.77 ± 0.13 | −3.42 ± 0.13 |
| WB89_1024 | 238.959 | −1.684 | 9.2 | 15.4 | 107 | 24.3 ± 4.4 | 3.58 ± 0.18 | 0.04 ± 0.15 | −4.04 ± 0.15 |
| WB89_890 | 212.282 | −0.617 | 6.4 | 14.3 | 120 | 27.2 ± 2.2 | 3.69 ± 0.13 | 0.02 ± 0.10 | −4.23 ± 0.10 |
| WB89_858 | 213.192 | −3.325 | 6.9 | 14.8 | 91 | 25.5 ± 0.4 | 3.37 ± 0.05 | −0.22 ± 0.09 | −4.22 ± 0.08 |
| WB89_1125 | 256.151 | −1.375 | 9.7 | 14.3 | 76 | 19.5 ± 1.8 | 3.09 ± 0.13 | 0.22 ± 0.11 | −4.01 ± 0.11 |
| WB89_879 | 214.931 | −2.719 | 6.9 | 14.7 | 99 | 26.5 ± 5.9 | 3.42 ± 0.29 | −0.19 ± 0.17 | −4.26 ± 0.17 |
| WB89_896 | 215.888 | −2.010 | 7.9 | 15.6 | 108 | 23.7 ± 4.4 | 3.50 ± 0.16 | −0.07 ± 0.16 | −4.18 ± 0.16 |
| WB89_856 | 213.098 | −3.561 | 7.7 | 15.6 | 114 | 26.3 ± 2.3 | 3.79 ± 0.15 | 0.24 ± 0.11 | −4.07 ± 0.10 |
| WB89_1126 | 257.508 | −2.252 | 10.6 | 15.0 | 53 | 24.4 ± 6.8 | 3.30 ± 0.31 | −0.15 ± 0.21 | −4.11 ± 0.21 |
| WB89_1006 | 235.686 | −1.246 | 8.1 | 14.7 | 110 | 28.5 ± 5.3 | 3.99 ± 0.27 | 0.24 ± 0.15 | −3.95 ± 0.15 |
| WB89_1008 | 236.999 | −1.838 | 8.8 | 15.2 | 114 | 19.8 ± 0.7 | 3.19 ± 0.06 | 0.24 ± 0.09 | −4.05 ± 0.08 |
| WB89_789 | 195.820 | −0.567 | 12.0 | 20.3 | 109 | 23.2 ± 3.1 | 4.09 ± 0.20 | 0.81 ± 0.13 | −3.56 ± 0.13 |
| WB89_1066 | 245.103 | −0.993 | 9.8 | 15.4 | 87 | 16.9 ± 0.2 | 2.85 ± 0.03 | 0.35 ± 0.08 | −3.91 ± 0.08 |
| WB89_1023 | 238.772 | −1.810 | 10.3 | 16.4 | 54 | 24.6 ± 5.0 | 3.09 ± 0.28 | −0.31 ± 0.17 | −4.30 ± 0.16 |
| WB89_1080 | 249.599 | −2.075 | 13.1 | 17.9 | 120 | 21.8 ± 0.6 | 3.81 ± 0.05 | 0.67 ± 0.08 | −4.25 ± 0.08 |
| WB89_873 | 215.599 | −3.414 | 7.1 | 14.9 | 114 | 21.2 ± 1.4 | 3.22 ± 0.10 | 0.12 ± 0.10 | −4.18 ± 0.10 |
| G237.32–1.28 | 237.320 | −1.280 | 8.7 | 15.1 | 114 | 31.4 ± 11.8 | 4.51 ± 0.42 | 0.50 ± 0.23 | −3.80 ± 0.23 |
| G233.38–1.60 | 233.380 | −1.600 | 8.7 | 15.4 | 120 | 12.1 ± 1.0 | 1.82 ± 0.09 | −0.04 ± 0.13 | −4.53 ± 0.13 |
| G229.76–0.44 | 229.760 | −0.440 | 8.4 | 15.3 | 120 | 13.9 ± 0.4 | 2.13 ± 0.05 | −0.01 ± 0.09 | −4.54 ± 0.09 |
| G235.35–1.74 | 235.350 | −1.690 | 9.3 | 15.8 | 120 | 18.1 ± 0.3 | 2.61 ± 0.04 | −0.04 ± 0.08 | −4.53 ± 0.08 |
| G233.76–1.25 | 233.760 | −1.250 | 8.7 | 15.3 | 117 | 13.9 ± 3.7 | 2.38 ± 0.15 | −0.03 ± 0.27 | −4.49 ± 0.27 |
Notes.
(a)
Calculated using the Brand & Blitz (1993) rotation curve.
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