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Trapping and desorption of complex organic molecules in water at 20 K
Author(s) -
Daren J. Burke,
Fabrizio Puletti,
Paul Woods,
S. Viti,
Ben Slater,
Wendy A. Brown
Publication year - 2015
Publication title -
the journal of chemical physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.071
H-Index - 357
eISSN - 1089-7690
pISSN - 0021-9606
DOI - 10.1063/1.4934264
Subject(s) - glycolaldehyde , desorption , thermal desorption , chemistry , molecule , chemical physics , interstellar ice , adsorption , sublimation (psychology) , astrochemistry , formate , intermolecular force , computational chemistry , astrobiology , interstellar medium , organic chemistry , astrophysics , physics , psychology , galaxy , psychotherapist , catalysis
The formation, chemical, and thermal processing of complex organic molecules (COMs) is currently a topic of much interest in interstellar chemistry. The isomers glycolaldehyde, methyl formate, and acetic acid are particularly important because of their role as pre-biotic species. It is becoming increasingly clear that many COMs are formed within interstellar ices which are dominated by water. Hence, the interaction of these species with water ice is crucially important in dictating their behaviour. Here, we present the first detailed comparative study of the adsorption and thermal processing of glycolaldehyde, methyl formate, and acetic acid adsorbed on and in water ices at astrophysically relevant temperatures (20 K). We show that the functional group of the isomer dictates the strength of interaction with water ice, and hence the resulting desorption and trapping behaviour. Furthermore, the strength of this interaction directly affects the crystallization of water, which in turn affects the desorption behaviour. Our detailed coverage and composition dependent data allow us to categorize the desorption behaviour of the three isomers on the basis of the strength of intermolecular and intramolecular interactions, as well as the natural sublimation temperature of the molecule. This categorization is extended to other C, H, and O containing molecules in order to predict and describe the desorption behaviour of COMs from interstellar ices.

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