Formation and Dissociation of N3 in Icy N2 with Far-ultraviolet Light

被引:5
|
作者
Lo, Jen-Iu [1 ]
Chou, Sheng-Lung [1 ]
Peng, Yu-Chain [1 ]
Lu, Hsiao-Chi [1 ]
Cheng, Bing-Ming [1 ]
机构
[1] Natl Synchrotron Radiat Res Ctr, 101 Hsin Ann Rd,Hsinchu Sci Pk, Hsinchu 30076, Taiwan
来源
ASTROPHYSICAL JOURNAL | 2019年 / 877卷 / 01期
关键词
astrochemistry; ISM: molecules; methods: laboratory: solid state; molecular processes; ultraviolet: ISM; SOLID NITROGEN; SPECTRA; PHOTODISSOCIATION; PHOTOLYSIS; METHANE; SURFACE; PLUTO;
D O I
10.3847/1538-4357/ab18f6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
During photoexcitation of icy N-2 at 121.6 nm from a synchrotron source, emission lines in the vibronic progression of the Vegard-Kaplan system, A (3)Sigma(+)(u) -> X-2(1)Sigma(+)(g), for N-2 were concurrently observed in the wavelength range 210-430 nm; emission lines of N (P-2 -> D-2) and N (D-2 -> S-4) were recorded in the wavelength range 460-1100 nm. After irradiation of icy N-2 at 121.6 nm, the characteristic infrared absorption lines of N(3 )radical in vibrational mode nu(3) appeared at 1652.6 and 1657.8 cm(-1). When the irradiated icy sample containing N-3 radical was subsequently subjected to photolysis at 190 nm, only emission from N (D-2 -> S-4) was concurrently recorded; the IR absorption lines of N-3 vanished. The result indicates that N-3 radical in icy N-2 can be dissociated into the N (D-2) atom and N-2 (X (1)Sigma(+)(g)) molecule with light at 190 nm. Our work thus has ramifications for nitrogen transformation in cold astrophysical environments.
引用
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页数:5
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