Table 2
Best-fitting column densities, excitation temperatures, and D/H ratios of CH3OD toward IRAS 16293-2422 B.
Best-fitting parameters | IRAS 16293-2422 B |
---|---|
Fitting υt = 0 and 1 together | |
Tex (K) | 190 ± 19 |
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(3.25 ± 0.65) × 1016 |
D/H of CH3OH | (3.2 ± 0.9) × 10−3 |
# lines | 97 |
Eup range (K) | 124 − 2969 |
Fitting solely υt = 0 | |
Tex (K) | 205 ± 21 |
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(2.52 ± 0.50) × 1016 |
D/H of CH3OH | (2.5 ± 0.7) × 10−3 |
# lines | 46 |
Eup range (K) | 124 − 2969 |
Fitting solely υt = 1 | |
Tex (K) | 163 ± 16 |
![]() |
(4.01 ± 0.80) × 1016 |
D/H of CH3OH | (4.0 ± 1.0) × 10−3 |
# lines | 51 |
Eup range (K) | 332 − 2287 |
Notes. Top part contains the best-fitting column density and excitation temperature of CH3OD obtained during simultaneous fitting of these two parameters for both υt = 0 and 1 states together and the associated D/H ratio. We note that the statistical correction on the D/H ratio for the case of deuteration in the hydroxy group is one (Appendix C of Drozdovskaya et al. 2022; see also Manigand et al. 2019). The fitting has also been executed for the two υt states separately, for which the corresponding derived column densities and D/H ratios are the middle and lower parts, respectively. The second column contains the values for the one-beam offset position in the SW direction from IRAS 16293-2422 B (0.5″ or 70 au away from the dust peak of B). For the calculations of D/H ratios, the adopted methanol column densities is (1.0 ± 0.2) × 1019 cm−2 (Jørgensen et al. 2018). The stated errors on N and Tex are assumed 20% and 10% errors, respectively. The errors derived with the MCMC routine in this work are much smaller (we refer to Drozdovskaya et al. (2022) for a discussion about that). For each of the three fitting scenarios, the number of lines with unique frequencies used for the fitting and the Eup range spanned by these lines are also provided.
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