Molecular Line Opacity of LiCl in the Mid‐Infrared Spectra of Brown Dwarfs

  • Weck P
  • Schweitzer A
  • Kirby K
  • et al.
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Abstract

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.

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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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