ExoMol line lists - III. An improved hot rotation-vibration line list for HCN and HNC

被引:204
作者
Barber, R. J. [1 ]
Strange, J. K. [1 ]
Hill, C. [1 ]
Polyansky, O. L. [1 ]
Mellau, G. Ch. [2 ]
Yurchenko, S. N. [1 ]
Tennyson, Jonathan [1 ]
机构
[1] UCL, Dept Phys & Astron, London WC1E 6BT, England
[2] Univ Giessen, Phys Chem Inst, D-35392 Giessen, Germany
基金
英国工程与自然科学研究理事会;
关键词
molecular data; opacity; astronomical data bases: miscellaneous; planets and satellites: atmospheres; stars: low-mass; NU(1) BAND SYSTEM; AB-INITIO; MODEL ATMOSPHERES; SYNTHETIC SPECTRA; CARBON STARS; C/O RATIO; SPECTROSCOPY; SURFACES; WATER; MOLECULES;
D O I
10.1093/mnras/stt2011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A revised rotation-vibration line list for the combined hydrogen cyanide (HCN)/hydrogen isocyanide (HNC) system is presented. The line list uses ab initio transition intensities calculated previously and extensive data sets of recently measured experimental energy levels. The resulting line list has significantly more accurate wavelengths than previous ones for these systems. An improved value for the separation between HCN and HNC is adopted, leading to an approximately 25 per cent lower predicted thermal population of HNC as a function of temperature in the key 2000 to 3000 K region. Temperature-dependent partition functions and equilibrium constants are presented. The line lists are validated by comparison with laboratory spectra and are presented in full as supplementary data to the article and at www.exomol.com.
引用
收藏
页码:1828 / 1835
页数:8
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