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

Author
WECK, P. F1 ; SCHWEITZER, A2 ; KIRBY, K3 ; HAUSCHILDT, P. H2 ; STANCIL, P. C4
[1] Department of Chemistry, University of Nevada at Las Vegas, 4505 Maryland Parkway, Las Vegas, NV 89154-4003, United States
[2] Hamburger Sternwarte, Universitaet Hamburg, Gojenbergsweg, 21029 Hamburg, Germany
[3] Institute for Theoretical Atomic, Molecular, and Optical Physics, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, United States
[4] Department of Physics and Astronomy and Center for Simulational Physics, University of Georgia, Athens, GA 30602-2451, United States
Source

The Astrophysical journal. 2004, Vol 613, Num 1, pp 567-571, 5 p ; 1 ; ref : 26 ref

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Abondance élément Atmosphère stellaire Energie transition Etoile type avancé Force oscillateur Interaction configuration Lithium chlorure Naine brune Opacité Processus moléculaire Spectre IR Transition rovibrationnelle
Keyword (en)
Element abundance Stellar atmospheres Transition energy Late type stars Oscillator strengths Configuration interaction Lithium chlorides Brown dwarf stars Opacity Molecular process Infrared spectra Rovibrational transition
Keyword (es)
Energía transición Proceso molecular Transición rovibracional
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C20 Normal stars (by class): general or individual / 001E03C20V Low luminosity stars, subdwarfs, and brown dwarfs

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C30 Variable and peculiar stars (including novae) / 001E03C30K Rr lyrae stars. Rv tauri and pv telescopii variables

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16227269

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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