Formation of complex organic molecules in cold objects: the role of gas phase reactions
Nadia Balucani, Cecilia Ceccarelli, Vianney Taquet

TL;DR
This paper presents a new gas-phase chemical model explaining the formation of complex organic molecules like methyl formate and dimethyl ether in cold interstellar environments, challenging the traditional grain-surface chemistry dominance.
Contribution
The study introduces a gas-phase reaction pathway for complex organic molecule formation in cold environments, supported by observational data and explaining correlations between molecules.
Findings
The model reproduces observed abundances in L1544.
Gas-phase reactions significantly contribute to complex molecule formation.
Correlation between DME and MF explained by the model.
Abstract
While astrochemical models are successful in reproducing many of the observed interstellar species, they have been struggling to explain the observed abundances of complex organic molecules. Current models tend to privilege grain surface over gas phase chemistry in their formation. One key assumption of those models is that radicals trapped in the grain mantles gain mobility and react on lukewarm (>30 K) dust grains. Thus, the recent detections of methyl formate (MF) and dimethyl ether (DME) in cold objects represent a challenge and may clarify the respective role of grain surface and gas phase chemistry. We propose here a new model to form DME and MF with gas phase reactions in cold environments, where DME is the precursor of MF via an efficient reaction overlooked by previous models. Furthermore, methoxy, a precursor of DME, is also synthetized in the gas phase from methanol, which is…
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