Table A.5
Column densities, expected C18O abundances and gas-to-dust ratios for the subsample of the TOP100 selected for this work.
Source | NC18O a |
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γ | γbf | NH2 b |
[10x cm-2] | [10-8] | [1022 cm-2] | |||
|
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AGAL010.472+00.027 | 16.66 ± 0.04 |
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AGAL010.624–00.384 | 17.16 ± 0.05 |
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AGAL012.804–00.199 | 17.01 ± 0.04 |
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AGAL013.658–00.599 | 16.05 ± 0.04 |
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AGAL015.029–00.669 | 16.87 ± 0.07 |
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AGAL019.882–00.534 | 16.21 ± 0.06 |
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AGAL028.861+00.066 | 16.50 ± 0.04 |
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AGAL030.818–00.056 | 16.39 ± 0.10 |
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AGAL031.412+00.307 | 16.64 ± 0.04 |
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AGAL034.258+00.154 | 17.02 ± 0.05 |
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AGAL034.401+00.226 | 16.43 ± 0.05 |
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AGAL034.411+00.234 | 16.03 ± 0.04 |
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AGAL034.821+00.351 | 16.24 ± 0.05 |
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AGAL035.197–00.742 | 16.35 ± 0.04 |
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AGAL037.554+00.201 | 16.14 ± 0.04 |
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AGAL043.166+00.011 | 17.28 ± 0.05 |
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AGAL049.489–00.389 | 17.15 ± 0.06 |
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AGAL053.141+00.069 | 16.27 ± 0.04 |
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AGAL059.782+00.066 | 16.03 ± 0.04 |
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AGAL301.136–00.226 | 16.63 ± 0.04 |
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AGAL305.209+00.206 | 16.50 ± 0.05 |
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AGAL305.562+00.014 | 16.56 ± 0.09 |
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AGAL309.384–00.134 | 16.25 ± 0.12 |
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AGAL310.014+00.387 | 16.21 ± 0.08 |
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AGAL313.576+00.324 | 16.22 ± 0.09 |
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AGAL316.641–00.087 | 15.81 ± 0.08 |
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AGAL326.661+00.519 | 16.42 ± 0.08 |
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AGAL327.119+00.509 | 16.35 ± 0.08 |
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AGAL327.293–00.579 | 17.11 ± 0.08 |
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AGAL327.393+00.199 | 15.92 ± 0.08 |
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AGAL328.809+00.632 | 17.04 ± 0.08 |
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AGAL329.066–00.307 | 15.71 ± 0.08 |
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AGAL330.879–00.367 | 16.98 ± 0.06 |
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AGAL330.954–00.182 | 17.24 ± 0.07 |
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AGAL332.094–00.421 | 16.56 ± 0.05 |
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AGAL332.826–00.549 | 17.13 ± 0.07 |
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AGAL333.134–00.431 | 17.10 ± 0.06 |
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AGAL333.284–00.387 | 16.81 ± 0.09 |
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AGAL333.314+00.106 | 16.10 ± 0.09 |
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AGAL333.604–00.212 | 16.86 ± 0.06 |
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AGAL337.406–00.402 | 16.98 ± 0.08 |
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AGAL337.704–00.054 | 16.65 ± 0.08 |
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AGAL337.916–00.477 | 17.09 ± 0.06 |
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AGAL339.623–00.122 | 16.20 ± 0.08 |
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AGAL340.746–01.001 | 16.02 ± 0.08 |
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AGAL341.217–00.212 | 16.24 ± 0.07 |
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AGAL343.128–00.062 | 16.77 ± 0.07 |
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AGAL345.003–00.224 | 16.61 ± 0.08 |
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AGAL345.488+00.314 | 16.79 ± 0.05 |
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AGAL345.504+00.347 | 16.72 ± 0.08 |
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AGAL345.718+00.817 | 16.11 ± 0.09 |
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AGAL351.161+00.697 | 16.71 ± 0.07 |
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AGAL351.244+00.669 | 16.93 ± 0.07 |
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AGAL351.416+00.646 | 16.99 ± 0.10 |
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AGAL351.581–00.352 | 16.88 ± 0.04 |
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AGAL351.774–00.537 | 17.13 ± 0.06 |
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AGAL353.409–00.361 | 16.93 ± 0.08 |
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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.
Calculated multiplying the measured C17O column density by a factor of 4 (see Giannetti et al. 2014).
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