The chemistry of multiply deuterated species in cold, dense interstellar cores

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Testing grain surface chemistry : a survey of deuterated formaldehyde and methanol in low-mass Class 0 protostars (2006, background): “Models of formaldehyde fractionation in prestellar cores –whose chemical and physical conditions are similar to those in the outer cold envelopes of Class 0 sources (Maret et al. 2004; Jørgensen et al. 2005)– seem approximatively to reproduce the observed ratios (Roberts et al. 2004).”
Probing the Evolutionary Status of Starless Cores through N2H+ and N2D+ Observations (2004, background): “…models where a population of smaller grains is present or where an MRN size distribution of dust particles is considered; and (3) the use of UMIST rates, which produce Hþ3 and analogs more efficiently than the ‘‘New Standard Model’’ from Ohio State University (for details see Roberts et al. 2004).”
The importance of the ortho:para H2 ratio for the deuteration of molecules during pre-protostellar collapse (2006, background): “The related reaction networks have been considered in detail by several authors (Roberts et al. 2003, 2004; Roueff et al. 2005).”