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Table 1

Measured FIR intensities of B207 and derived physical properties.

Region 160 μm 250 μm 350 μm 500 μm T N(H) M(H) TAbel NAbel(H)
MJy/sr MJy/sr MJy/sr MJy/sr K 1021 cm-2 M K 1021 cm-2

1(south) 1.75 2.66 1.97 1.01
2 0.30 3.28 2.21 1.36
3 9.21 15.3 9.54 5.00 14.1 2.46 0.04 11.6 4.01
4 28.7 45.6 31.3 15.1 13.6 8.13 0.15 11.1 13.7
5 47.8 79.5 57.6 28.9 13.0 17.3 0.32 10.6 29.9
6 63.8 121 101 49.1 12.0 35.9 0.66 10.1 58.5
7 69.8 151 136 78.2 11.1 71.6 1.31 9.40 117
8(core) 117 201 170 89.4 11.7 69.6 1.27 10.1 107
9 115 182 135 63.9 12.9 38.5 0.70 10.6 66.0
10 58.5 99.8 74.0 34.4 13.0 20.6 0.38 11.1 31.2
11 44.1 78.1 54.8 25.6 13.4 14.1 0.26 11.6 20.5
12 27.4 57.3 39.9 18.9 13.3 10.6 0.19 12.7 12.0
13 20.3 41.5 27.6 13.3 13.7 7.01 0.13 13.3 7.50
14 13.4 32.7 21.1 10.1 13.8 5.20 0.09
15(north) 11.7 28.2 18.2 8.48 13.8 4.35 0.08

Notes. Temperature, column density and mass for regions 1 and 2 were not estimated since they are outside of the globule in the diffuse sky region. The column density, N(H), and mass, M(H), are calculated for each region using the AMM and AMMI dust mass opacity at 500 μm from Köhler et al. (2015). The temperature, TAbel, and column density, NAbel(H), are the temperature and the corresponding column density, respectively, estimated from the Abel inversion method.

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