Molecular Line Opacity of LiCl in the Mid‐Infrared Spectra of Brown Dwarfs
Author(s) -
Philippe F. Weck,
A. Schweitzer,
K. Kirby,
P. H. Hauschildt,
P. C. Stancil
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/423029
Subject(s) - opacity , rotational–vibrational spectroscopy , brown dwarf , spectral line , physics , ground state , atomic physics , line (geometry) , absorption spectroscopy , quantum number , astrophysics , computational physics , stars , astronomy , optics , geometry , mathematics
We present a complete line list for the X 1Sigma+ electronic ground state ofLiCl computed using fully quantum-mechanical techniques. This list includestransition energies and oscillator strengths in the spectral region0.3-39,640.7 cm-1 for all allowed rovibrational transitions in absorptionwithin the electronic ground state. The calculations were performed using anaccurate hybrid potential constructed from a spectral inversion fit ofexperimental data and from recent multi-reference single- and double-excitationconfiguration interaction calculations. The line list was incorporated into thestellar atmosphere code PHOENIX to compute spectra for a range of young to oldT dwarf models. The possibility of observing a signature of LiCl in absorptionnear 15.8 microns is addressed and the proposal to use this feature to estimatethe total lithium elemental abundance for these cool objects is discussed.Comment: 8 pages, 2 figures, 1 table. Accepted for publication in ApJ 613, Sept. 20 200
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