Formation of Nascent Product N2O from the Irradiation of O2 in Icy N2

被引:7
|
作者
Lo, Jen-Iu [1 ]
Chou, Sheng-Lung [1 ]
Peng, Yu-Chain [1 ]
Lu, Hsiao-Chi [1 ]
Ogilvie, J. F. [2 ,3 ]
Cheng, Bing-Ming [1 ]
机构
[1] Natl Synchrotron Radiat Res Ctr, 101 Hsin Ann Rd,Hsinchu Sci Pk, Hsinchu 30076, Taiwan
[2] Simon Fraser Univ, Dept Math, Burnaby, BC V5A1S6, Canada
[3] Univ Costa Rica, Escuela Quim, Ciudad Univ Rodrigo Facio, San Jose 115012060, Costa Rica
来源
ASTROPHYSICAL JOURNAL | 2018年 / 864卷 / 01期
关键词
astrobiology; astrochemistry; ISM: molecules; molecular processes; SOLAR-SYSTEM BODIES; SOLID N-2; MOLECULES; ICES; ANALOGS; PHOTOCHEMISTRY; HYDROCARBONS; PHOTOLYSIS; RADIATION; MIXTURES;
D O I
10.3847/1538-4357/aad55e
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Products O-3, N, NO, NO2, N2O, c-(NO)(2), and excited states of O-2 were detected after the photolysis of solid O-2 in icy N-2 near 4 K with radiation at 200 nm. The temporal profiles of these products enable the derivation of a mechanism for the photochemical reactions in this system: dissociation of O-2 first-generated (OP)-P-3 that reacted with nearby N-2 to yield N2O. Other products resulted from the secondary photolysis of N2O and the reactions of O with N2O. The reaction of O with O-2 to form O-3 was impeded by the small concentration of the latter, which requires substantial migration through the N-2 lattice. However, sufficient O-3 was eventually formed to enable detection either directly from O coming from O-2 or indirectly through N2O. These results enhance our understanding of the evolution of the transformation of oxygen and nitrogen in irradiated ices and have possible astrophysical applications.
引用
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页数:6
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