Molecular line opacity of LiCl in the mid-infrared spectra of brown dwarfs

被引:19
作者
Weck, PF
Schweitzer, A
Kirby, K
Hauschildt, PH
Stancil, PC
机构
[1] Univ Nevada, Dept Chem, Las Vegas, NV 89154 USA
[2] Univ Hamburg, D-21029 Hamburg, Germany
[3] Harvard Smithsonian Ctr Astrophys, Inst Theoret Atom Mol & Opt Phys, Cambridge, MA 02138 USA
[4] Univ Georgia, Dept Phys & Astron, Athens, GA 30602 USA
[5] Univ Georgia, Ctr Simulat Phys, Athens, GA 30602 USA
关键词
molecular data; stars : atmospheres; stars : late-type;
D O I
10.1086/423029
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a complete line list for the X(1)Sigma(+) electronic ground state of (LiCl)-Li-7-Cl-35, 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 mum 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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页码:567 / 571
页数:5
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