Open Access
Table B.1.
Observed line parameters of the HOCHCHCHO transitions identified towards IRAS 16293 B.
Transition | Frequency | Integrated flux | Imax | vLSR | FWHM |
---|---|---|---|---|---|
![]() ![]() |
(MHz) | (Jy beam−1 km s−1) | (Jy beam−1) | (km s−1) | (km s−1) |
17 17 0 1 - 16 16 1 1 | 329184.3 | 0.024 | 0.028 ± 0.004 | 2.64 ± 0.05 | 0.72 ± 0.11 |
17 17 1 1 - 16 16 0 1 | 329184.3 | ||||
21 14 7 0 - 20 13 8 0 | 330826.2 | 0.037 | 0.022 ± 0.003 | 2.76 ± 0.08 | 1.61 ± 0.21 |
21 14 8 0 - 20 13 7 0 | 330826.5 | ||||
20 15 5 0 - 19 14 6 0† | 333154.6 | 0.045 | 0.069 ± 0.007 | 2.66 ± 0.03 | 0.63 ± 0.07 |
20 15 6 0 - 19 14 5 0† | 333154.6 | ||||
19 16 3 0 - 18 15 4 0 | 335375.8 | 0.032 | 0.045 ± 0.006 | 2.88 ± 0.05 | 0.70 ± 0.11 |
19 16 4 0 - 18 15 3 0 | 335375.8 | ||||
19 16 3 1 - 18 15 4 1 | 335563.8 | 0.016 | 0.024 ± 0.005 | 2.95 ± 0.05 | 0.51 ± 0.12 |
19 16 4 1 - 18 15 3 1 | 335563.8 | ||||
25 12 13 0 - 24 11 14 0† | 341865.3 | 0.014 | 0.025 ± 0.005 | 2.60 ± 0.04 | 0.47 ± 0.10 |
20 16 4 1 - 19 15 5 1‡ | 344235.8 | 0.020 | 0.033 ± 0.003 | 2.81 ± 0.09 | 0.76 ± 0.19 |
20 16 5 1 - 19 15 4 1‡ | 344235.8 | ||||
24 14 10 1 - 23 13 11 1† | 356301.7 | 0.032 | 0.040 ± 0.006 | 2.87 ± 0.06 | 0.78 ± 0.14 |
19 18 1 1 - 18 17 2 1‡ | 357554.9 | < 0.067 | 0.026 ± 0.003 | 2.89 ± 0.15 | 1.10 ± 0.35 |
19 18 2 1 - 18 17 1 1‡ | 357554.9 | ||||
22 16 7 1 - 21 15 6 1‡ | 361541.5 | < 0.045 | 0.023 ± 0.031 | [2.7] | [0.7] |
22 16 6 1 - 21 15 7 1‡ | 361541.5 | ||||
29 12 18 1 - 28 11 17 1† | 362238.2 | 0.019 | 0.020 ± 0.003 | 2.62 ± 0.07 | 0.96 ± 0.16 |
13 12 1 1 - 12 11 2 1†‡ | 239460.6 | < 0.020 | 0.008 ± 0.003 | [2.7] | [0.7] |
13 12 2 1 - 12 11 1 1†‡ | 239460.6 | ||||
18 9 10 0 - 17 8 9 0 | 247531.2 | 0.012 | 0.011 ± 0.001 | 2.59 ± 0.06 | 1.19 ± 0.17 |
13 13 0 1 - 12 12 1 1 | 250459.9 | 0.012 | 0.015 ± 0.001 | 2.43 ± 0.05 | 0.87 ± 0.13 |
13 13 1 1 - 12 12 0 1 | 250459.9 |
Note: The values in square brackets are assumed. The uncertainties correspond to the fit uncertainties only. † These lines could be partially blended with unknown species. ‡ A double Gaussian is used to fit the observations.
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