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This article has an erratum: [https://doi.org/10.1051/0004-6361/201935428e]


Table 5

Deuterium fractionation of selected (complex) organic molecules toward Sgr B2(N2) compared to predictions of astrochemical models.

Molecule Statusa [XD]/[XH]

N2b T14c A12d
% % %

CH2DCN d 0.38 3.6–0.15 2.3–6.3
CH2DCH2CN (oop) t 0.05
CH2DCH2CN (ip) n <0.024
CH3CHDCN t 0.05
cis-CHDCHCN n <0.8
trans-CHDCHCN n <0.8
CH2CDCN n <0.5
DC3N t 0.09 5.4–1.1
CH2DOH t 0.12 5.5–0.51 2.4–2.4e
CH3OD n <0.07 3.5–0.3 e
CH3CH2OD n <1.5
CH3CHDOH n <1.5
CH2DCH2OH (oop) n <1.5
CH2DCH2OH (ip) n <1.0
CH2DOCHO (oop) n <2.0 14–0.43f
CH2DOCHO (ip) n <0.6 7–0.22f

Notes. The notations oop and ip describe the position of the deuterium and stand for out of plane and in plane, respectively.

(a)

d: detection, t: tentative detection, n: nondetection.

(b)

Deuterium fractionation measured toward Sgr B2(N2).

(c)

Deuterium fractionation predicted by the model of Taquet et al. (2014) in the hot corino at the beginning and end of the Class 0 phase.

(d)

Deuterium fractionation predicted by the model of Aikawa et al. (2012) in the hot corino at the beginning and end of the Class 0 phase.

(e)

The model of Aikawa et al. (2012) was not designed to predict the abundance ratios of deuterated isomers: it assumes statistical branching ratios.

(f)

The model of Taquet et al. (2014) does not distinguish between the in-plane and out-of-plane conformers. The values listed here assume a statistical distribution (2:1).

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