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Table A.4

Column densities, expected C18O abundances, gas-to-dust ratios and radial velocities for the far outer Galaxy sample.

Source NC18O γ γbf NH2 b VLSR
[10x cm-2 ] [10-8] [1022 cm-2 ] [km s-1]

WB89_898 15.14 ± 0.06 63.35
WB89_986 14.71 ± 0.04 70.57
WB89_909 15.83 ± 0.08 50.06/52.40a
WB89_1024 14.88 ± 0.08 82.42
WB89_890 14.55 ± 0.09 46.29/47.59a
WB89_858 14.78 ± 0.09 49.34
WB89_1125 14.79 ± 0.04 86.08
WB89_879 14.04 ± 0.12 51.98
WB89_896 14.59 ± 0.08 57.55
WB89_856 15.01 ± 0.09 52.63
WB89_1126 14.80 ± 0.08 90.41
WB89_1006 14.67 ± 0.10 74.81
WB89_1008 14.52 ± 0.04 80.41
WB89_789 15.38 ± 0.07 34.24
WB89_1066 14.77 ± 0.04 87.01
WB89_1023 14.65 ± 0.08 88.74
WB89_1080 14.36 ± 0.06 105.92
WB89_873 14.20 ± 0.06 53.65
G237.32–1.28 15.01 ± 0.10 78.07
G233.38–1.60 13.67 ± 1.30 76.70
G229.76–0.44 13.98 ± 0.93 73.03
G235.35–1.74 14.42 ± 0.14 80.98
G233.76–1.25 14.23 ± 0.65 76.91

Notes. The uncertainties reported for each quantity are calculated using the limiting cases for the C18O abundance discussed in the text. The values of the gas-to-dust ratio obtained with the best-fit relation in Eq. (2) are reported in the γbf column.

(a)

Sources with multiple velocity components.

(b)

The surface density of gas is obtained multiplying NH2 by the mean molecular mass μmH.

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