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Table 4

PDR model results.

Model AV Star D θ nH I([C II]) I([O I] 63) I([O I] 145) I([O I] 63)/ I([O I] 145)/
(pc) (deg) (cm−3) (K km s−1) (K km s−1) (K km s−1) I([C II]) I([C II])
1027 10 O 5 V −13 0 9 × 103 26.43 1.74 0.53 0.066 0.020
1028 10 O 5 V 13 0 9 × 103 20.51 0.50 0.53 0.025 0.026
1029 10 O 5 V −15 30 9 × 103 26.04 1.33 0.40 0.051 0.015
1030 10 O 5 V 15 30 9 × 103 19.84 0.37 0.40 0.018 0.020
1031 10 O 5 V −26 60 9 × 103 21.88 0.41 0.11 0.019 0.005
1032 10 O 5V 26 60 9 × 103 15.81 0.10 0.11 0.006 0.007
1033 10 O 5V −15 30 4.5 × 104 22.48 2.35 0.69 0.105 0.031
1034 10 O 5V 15 30 4.5 × 104 20.85 1.42 0.69 0.068 0.033

Observed 13–32 1.4–4.0 3.6–4.4 0.08–0.14 0.11–0.33

Notes. Entries in the table are: model number, stellar type, distance (pc; negative and positive values imply front-side and back-side illumination, respectively), the [O I] 63 µm, [O I] 145 µm, and [C II] integrated line intensities (K km s−1), the [O I] 63 [C II] line ratio, and the [O I]/145 µm to [C II] line ratio. All models assume a turbulent velocity dispersion of 0.9 km s−1, as suggested by the observed [CII] line widths and face-on illumination.

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