Far-infrared spectroscopy of proteinogenic and other less common amino acids

被引:11
作者
Iglesias-Groth, S. [1 ,2 ]
Cataldo, F. [3 ,4 ]
机构
[1] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain
[2] Univ La Laguna, Dept Astrofis, Avda Francisco Sanchez, E-38200 San Cristobal la Laguna, Spain
[3] Actinium Chem Res Inst, Via Casilina 1626A, I-00133 Rome, Italy
[4] INAF Osservatorio Astrofis Catania, Via S Sofia 78, I-95123 Catania, Italy
关键词
astrochemistry; methods: laboratory: molecular; techniques: spectroscopic; infrared: general; INTERSTELLAR ICE ANALOGS; CIRCULARLY-POLARIZED LIGHT; TERAHERTZ SPECTROSCOPY; ULTRAVIOLET PHOTOLYSIS; COSMIC ABUNDANCES; ORGANIC-COMPOUNDS; MATRIX-ISOLATION; SPACE-TELESCOPE; HEAT BALANCES; AB-INITIO;
D O I
10.1093/mnras/sty1226
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Far-infrared spectroscopy is a powerful tool complementing the potential of mid-infrared spectroscopy for the search and identification of organic molecules in space. The far-infrared spectra of a total of 29 amino acids are reported in this study. In addition to the spectra of 20 common proteinogenic amino acids, spectra of a selection of nine non-proteinogenic amino acids are also reported, including the 2-aminoisobutyric acid or a-aminoisobutyric acid which, with glycine, form the most abundant amino acids found in meteorites. The present data base of 29 far-infrared spectra may serve as a reference in the search for amino acids in space environments, given the new opportunities that JWST offers for mid-and far-IR spectroscopy.
引用
收藏
页码:3430 / 3437
页数:8
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