Table 3.
CH2DOH/CH3OH and CH3OD/CH3OH values derived from 13CH3OH or .
Source | Region | CH2DOH/CH3OH |
(CH2DOH/CH3OH)corra |
CH3OD/CH3OH |
CH2DOH/CH3ODb | |||
---|---|---|---|---|---|---|---|---|
12C/13C | 16O/18O | 12C/13C | 16O/18O | 12C/13C | 16O/18O | |||
[%] | [%] | [%] | [%] | [%] | [%] | |||
NGC 6334 I | MM1 I | 0.11–0.32 | 0.06–0.07 | 0.04–0.11 | 0.02 | 1.07 | 0.36–0.61 | 0.16–0.19 |
MM1 II | 0.05–0.17 | 0.03–0.07 | 0.02–0.06 | 0.01–0.02 | 0.83 | 0.35–0.42 | 0.10–0.13 | |
MM1 III | 0.07–0.21 | 0.06–0.14 | 0.02–0.07 | 0.02–0.05 | 0.45 | 0.30 | 0.23–0.29 | |
MM1 IV | 0.04–0.16 | 0.03–0.07 | 0.01–0.05 | 0.01–0.03 | 0.53 | 0.25 | 0.12–0.19 | |
MM1 V | 0.09–0.20 | 0.04–0.09 | 0.03–0.07 | 0.01–0.03 | 0.50 | 0.22 | 0.25 | |
MM2 I | 0.11–0.34 | 0.13–0.20 | 0.04–0.11 | 0.04–0.07 | 0.44 | 0.27–0.50 | 0.38–0.50 | |
MM2 II | 0.03–0.08 | 0.03–0.06 | 0.01–0.03 | 0.01–0.02 | 0.39 | 0.30 | 0.15 | |
MM3 I | 0.05–0.11 | 0.04–0.10 | 0.08–0.04 | 0.01–0.03 | 0.27 | 0.24 | 0.25 | |
MM3 II | 0.05–0.13 | 0.04–0.11 | 0.02–0.04 | 0.01–0.04 | 0.32 | 0.27 | 0.23 | |
Sgr B2c | N2 | 0.12 | – | 0.04 | – | <0.07 | – | >1.8 |
Orion KLd,e | Compact Ridge | 0.58 ± 0.12 | – | 0.19 | – | 0.5 ± 0.1 | – | 1.2 ± 0.3 |
(0.08–0.13) | – | 0.03–0.04 | – | – | 0.7 ± 0.3 0.3f | |||
Orion Bg | HH 212 | 2.4 ± 0.4 | – | 0.8 ± 0.1 | – | – | – | – |
IRAS 16293–2422h | B | – | 7.1i | – | 2.4i | – | 1.8 | 3.9 |
Notes.
Ranges of CH2DOH/CH3OH and CH3OD/CH3OH correspond to the range in column density of 13CH3OH, and CH2DOH with and without blending. All CH2DOH/CH3OH values include the vibrational correction of 1.25 as well as the uncertainy in the line strength.
Corrected for statistical weight of the location of the substituted deuterium. For CH2DOH this value is 3, for CH3OD it is 1.
Includes vibration correction factor for CH2DOH of 1.457 at 300 K (see Sect. 2.2 of Jørgensen et al. 2017).
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