ExoMol molecular line lists - XXXVII. Spectra of acetylene

被引:93
作者
Chubb, Katy L. [1 ,2 ]
Tennyson, Jonathan [1 ]
Yurchenko, Sergei N. [1 ]
机构
[1] UCL, Dept Phys & Astron, London WC1E 6BT, England
[2] SRON Netherlands Inst Space Res, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands
基金
英国科学技术设施理事会;
关键词
molecular data; planets and Satellites: atmospheres; stars: atmosphere; stars: carbon; ROTATION-VIBRATION SPECTRUM; DYNAMIC-MODEL ATMOSPHERES; NEAR-INFRARED SPECTRA; CARBON STARS; ABSORPTION-SPECTRUM; SPECTROSCOPIC DATA; AGB STARS; CHEMISTRY; METHANE; CM(-1);
D O I
10.1093/mnras/staa229
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A new ro-vibrational line list for the ground electronic state of the main isotopologue of acetylene, (C2H2)-C-12, is computed as part of the ExoMol project. The aCeTY line list covers the transition wavenumbers up to 10 000 cm(-1) (lambda > 1 mu m), with lower and upper energy levels up to 12 000 and 22 000 cm(-1) considered, respectively. The calculations are performed up to a maximum value for the vibrational angular momentum, K-max = L-max = 16, and maximum rotational angular momentum, J = 99. Higher values of J were not within the specified wavenumber window. The aCeTY line list is considered to be complete up to 2200 K, making it suitable for use in characterizing high-temperature exoplanet or cool stellar atmospheres. Einstein-A coefficients, which can directly be used to calculate intensities at a particular temperature, are computed for 4.3 billion (4 347 381 911) transitions between 5 million (5 160803) energy levels. We make comparisons against other available data for (C2H2)-C-12, and demonstrate this to be the most complete line list available. The line list is available in electronic form from the online CDS and ExoMol data bases.
引用
收藏
页码:1531 / 1545
页数:15
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