A new model for brown dwarf spectra including accurate unified line shape theory for the Na I and K I resonance line profiles

Astronomy and Astrophysics

Volumn 411, Issue 3, 2003, Pages

  Allard, N F ^a,b   Allard, F ^c   Hauschildt, P H ^d   Kielkopf, J F ^e   Machin, L ^a,c  

^a CNRS   (France)

^b OBSERVATOIRE DE PARIS   (France)

^c CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^d UNIVERSITY OF HAMBURG   (Germany)

^e UNIVERSITY OF LOUISVILLE   (United States)

Author keywords

Brown dwarfs; Line: profiles; Radiation mechanisms: general; Stars: atmospheres

Indexed keywords

FOURIER TRANSFORMS; HELIUM; LIGHT ABSORPTION; METHANE; OPACITY; POTASSIUM; RESONANCE; SATELLITES; SODIUM; SPECTRUM ANALYSIS;

BOLTZMANN FACTOR; INTERNUCLEAR REGIONS; SHAPE THEORY;

ASTROPHYSICS;

EID: 0344082228     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031299     Document Type: Article

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