ExoMol line lists - LV: hyperfine-resolved molecular line list for vanadium monoxide (51V16O)

被引:7
|
作者
Bowesman, Charles A. [1 ]
Qu, Qianwei [1 ,2 ]
Mckemmish, Laura K. [3 ]
Yurchenko, Sergei N. [1 ]
Tennyson, Jonathan [1 ]
机构
[1] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
[2] Paul Scherrer Inst, CH-5232 Villigen, Switzerland
[3] Univ New South Wales, Sch Chem, Sydney 2052, Australia
基金
欧洲研究理事会;
关键词
molecular data; opacity; planets and satellites: atmospheres; planets and satellites: exoplanets; stars: atmospheres; HOT JUPITERS; TRANSMISSION SPECTRUM; EMISSION-SPECTROSCOPY; EQUILIBRIUM-CONSTANTS; ROTATIONAL STRUCTURE; PARTITION-FUNCTIONS; DIATOMIC-MOLECULES; THERMAL INVERSIONS; RADIATIVE-TRANSFER; V838; MONOCEROTIS;
D O I
10.1093/mnras/stae542
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The new hyperfine-resolved HyVO line lists for vanadium monoxide ((VO)-V-51-O-16) are presented. The new line list considers 15 electronic states and comprises almost 59 billion transitions between 3.4 million energy levels, up to 45 000 cm(-1). Empirical energy levels obtained through the Marvel procedure are used to update calculated values to experimental accuracy, making the line list well suited for high-resolution experiments. Machine learning is utilized to refine the energies of levels in important bands, where empirical values are not known. These updates allow for the accurate prediction of line positions in regions of astrophysical interest, particularly in strong rovibronic bands in the infrared and visible. Previously published ab initio transition dipole moment curves are adjusted based on experimental lifetime measurements, resulting in increased intensities in key regions. The line list covers levels up to F = 150 and is complete up to 5400 K, making it well suited for studies of ultra-hot Jupiter and M-type stellar atmospheres where VO is believed to be a strong source of opacities. The full line list is made available via www.exomol.com.
引用
收藏
页码:1321 / 1332
页数:12
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