Abstract
Experimental techniques of high-resolution infrared absorption spectroscopy are described with an emphasis on the modulated hollow-cathode discharge techniques. Among the recent results, the rq fundamental band of HOCS+ |iq — 3435.16 cm-1) and the X2IT and a4E” system of NH+ (t0 = 2903.17 cm-1 in X2II state, = 2544.30 cm-1 in a4E~ state, and A£(a4E_ —X2n) — 323.90 cm-1) are presented to illustrate the quality and type of information that the high-resolution ion spectroscopy can provide. Another topic discussed is the abundance ratio [HCO+]/[H O C +] as measured in the laboratory and its astrophysics implications. The measurement has been made possible by our recent detection of the rq fundamental band of HOC+ (iq, — 3268.03 cm""1). A rate-equation analysis was performed by assuming a reaction scheme to derive the rate constants of several key reactions.
Reference9 articles.
1. Kawaguchi & Amano (1987 s)
2. Brown etal. (1986)
3. Greubele et al. (1987 s)
4. Adams N. G. & Smith D. 1987 In Astrochemistry. IAU Symposium no. 120 (ed. M. 8. Vardya & S. P. Tarafdar) Dordrecht: Reidel.
5. An analysis of the O2+ First Negative band system
Cited by
31 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献