ExoMol line lists - L: high-resolution line lists of H3+, H2D+, D2H+, and D3+

被引:7
作者
Bowesman, Charles A. [1 ]
Mizus, Irina I. [2 ,3 ]
Zobov, Nikolay F. [3 ]
Polyansky, Oleg L. [1 ,3 ]
Sarka, Janos [4 ,5 ]
Poirier, Bill [4 ]
Pezzella, Marco [1 ]
Yurchenko, Sergei N. [1 ]
Tennyson, Jonathan [1 ]
机构
[1] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
[2] Holon Inst Technol, Golomb St 52, IL-5810201 Holon, Israel
[3] Russian Acad Sci, Inst Appl Phys, Ulyanov St 46, Nizhnii Novgorod 603950, Russia
[4] Texas Tech Univ, Dept Chem & Biochem, Lubbock, TX 79409 USA
[5] Eotvos Lorand Univ, Inst Chem, Pazmany Peter setany 1-A, H-1117 Budapest, Hungary
基金
美国国家科学基金会; 欧洲研究理事会;
关键词
molecular data; opacity; planets and satellites :atmospheres; stars : atmospheres; ISM :molecules; ROTATIONAL-VIBRATIONAL STATES; CAVITY RINGDOWN SPECTROSCOPY; SUBMILLIMETER-WAVE LINES; GRID-BASED APPLICATIONS; NU-3 FUNDAMENTAL BANDS; INFRARED-SPECTRUM; MOLECULAR-IONS; OVERTONE BAND; PARALLEL IMPLEMENTATION; LABORATORY OBSERVATION;
D O I
10.1093/mnras/stad050
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
New MiZo line lists are presented for the D2H+ and D-3(+) isotopologues of H-3(+) . These line lists plus the existing H-3(+) MiZATeP and the ST H2D+ line lists are updated using empirical energy levels generated using the MARVEL procedure for H-3(+) , H2D+, and D2H+, and effective Hamiltonian energies for D-3(+) for which there is significantly less laboratory data available. These updates allow accurate frequencies for far infrared lines for these species to be predicted. Assignments of the energy levels of H-3(+) and D-3(+) are extended using a combination of high accuracy variational calculations and analysis of transition intensities. All line lists are made av ailable via www.exomol.com .
引用
收藏
页码:6333 / 6348
页数:16
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