We present a complete line list for the X1Σ+ electronic ground state of 7Li35Cl, computed using fully quantum-mechanical techniques. This list includes transition energies and oscillator strengths in the spectral region 0.3-39,640.7 cm-1 for all allowed rovibrational transitions in absorption within the electronic ground state. The calculations were performed using an accurate hybrid potential constructed from a spectral inversion fit of experimental data and from recent multireference single- and double-excitation configuration interaction calculations. The line list was incorporated into the stellar atmosphere code PHOENIX to compute spectra for a range of young to old T dwarf models. The possibility of observing a signature of LiCl in absorption near 15.8 μm is addressed and the proposal to use this feature to estimate the total lithium elemental abundance for these cool objects is discussed.
CITATION STYLE
Weck, P. F., Schweitzer, A., Kirby, K., Hauschildt, P. H., & Stancil, P. C. (2004). Molecular Line Opacity of LiCl in the Mid‐Infrared Spectra of Brown Dwarfs. The Astrophysical Journal, 613(1), 567–571. https://doi.org/10.1086/423029
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