Interstellar ices as witnesses of star formation: selective deuteration of water and organic molecules unveiled
S. Cazaux, P. Caselli, M. Spaans

TL;DR
This study investigates the selective deuteration of water and organic molecules in interstellar ices during star formation, explaining observed variations through chemical modeling of ice formation and evolution.
Contribution
It introduces a detailed chemical model that explains the differential deuteration of water and organic molecules in star-forming environments.
Findings
Deuteration of formaldehyde depends on the gas D/H ratio during collapse.
Deuteration of water depends on dust temperature at ice formation.
Model reproduces observed deuterium fractionation in comets and star-forming regions.
Abstract
Observations of star forming environments revealed that the abundances of some deuterated interstellar molecules are markedly larger than the cosmic D/H ratio of 10-5. Possible reasons for this pointed to grain surface chemistry. How- ever, organic molecules and water, which are both ice constituents, do not enjoy the same deuteration. For example, deuterated formaldehyde is very abundant in comets and star forming regions, while deuterated water rarely is. In this article, we explain this selective deuteration by following the formation of ices (using the rate equation method) in translucent clouds, as well as their evolu- tion as the cloud collapses to form a star. Ices start with the deposition of gas phase CO and O onto dust grains. While reaction of oxygen with atoms (H or D) or molecules (H2) yields H2O (HDO), CO only reacts with atoms (H and D) to form H2CO (HDCO, D2CO). As a…
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