Oxygen line formation in late-F through early-K disk/halo stars. Infrared O I triplet and [O I] lines

Astronomy and Astrophysics

Volumn 402, Issue 1, 2003, Pages 343-359

  Takeda, Y ^a  

^a KOMAZAWA UNIVERSITY   (Japan)

Author keywords

Galaxy: abundances; Line: formation; Radiative transfer; Stars: late type; Stars: population II

Indexed keywords

ATMOSPHERIC CHEMISTRY; ATMOSPHERIC RADIATION; ATOMIC PHYSICS; CALCULATIONS; GALAXIES; MATHEMATICAL MODELS; NUMERICAL METHODS; OXYGEN;

ATMOSPHERIC PARAMETERS; NEUTRAL ATOMIC OXYGEN; RADIATIVE TRANSFER; STARS;

ASTROPHYSICS;

EID: 0038639336     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030217     Document Type: Article

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