Pathways to Glycine and Other Amino Acids in Ultraviolet-irradiated Astrophysical Ices Determined via Quantum Chemical Modeling
By D. Woon. 2002
169 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/25ae385aec2ed59b34c2cdbc647ae9ce39e52531
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Citations in the corpus
- Erratum: Detection of amino acetonitrile in Sgr B2(N) (2008, background): “On the other hand, Elsila et al. (2007) experim nted the UV-photolysis of an ice mixture of H2O, CH3OH, HCN, and NH3, and found with isotopic labeling techniques multiple pathways leading to the formation of amino acids.”
- A Combined Experimental and Theoretical Study on the Formation of the Amino Acid Glycine (NH2CH2COOH) and Its Isomer (CH3NHCOOH) in Extraterrestrial Ices (2005, methodology): “Woon (2002) utilized quantum chemical modeling of astrophysical ices.”
- Complex organic molecules in protoplanetary disks (2013, unknown): “Recently, Garrod (2013) investigated the formation of glycine in hot cores via grain-surface radical-radical reactions, i.e., an extension to the reaction scheme used here, incorporating the ice chemistry proposed in Woon (2002) to describe the formation of glycine in UV-irradiated ices.”
- A THREE-PHASE CHEMICAL MODEL OF HOT CORES: THE FORMATION OF GLYCINE (2013, methodology): “7) on the ice surface, by the route s ggested by Woon (2002).”
- Mechanisms of Amino Acid Formation in Interstellar Ice Analogs (2007, methodology): “In contrast, a radical-radical mechanism in which dehydrogenation of CH3OH and H2O combined with hydrogenation of HCN forms glycine was proposed in Woon (2002).”
- Interstellar Ice: The Infrared Space Observatory Legacy (2004, background): “…searches have focused on the gas phase (see Snyder 1997 for a review), but recent work has emphasized the possibility that they might be a minor constituent of ices that have been subjected to UV INTERSTELLAR ICE 61No. 1, 2004 photolysis (Bernstein et al. 2002; Munoz Caro et al. 2002; Woon 2002).”