The non-LTE line formation of neutral carbon in late-type stars

Astronomy and Astrophysics

Volumn 458, Issue 3, 2006, Pages 899-914

  Fabbian, D ^a   Asplund, M ^a   Carlsson, M ^b   Kiselman, D ^c  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b UNIVERSITY OF OSLO   (Norway)

^c ALBANOVA UNIVERSITY CENTER   (Sweden)

Author keywords

Galaxy: abundances; Galaxy: evolution; Line: formation; Stars: abundances; Stars: late type

Indexed keywords

ATMOSPHERIC MOVEMENTS; CARBON; CODES (SYMBOLS); ERROR CORRECTION; MATHEMATICAL MODELS; STATISTICAL METHODS; THERMODYNAMICS;

GALACTIC CHEMICAL EVOLUTION MODELS; NEUTRAL CARBON; NON-LOCAL THERMODYNAMIC EQUILIBRIUM (NON-LTE);

GALAXIES;

EID: 33750738595     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065763     Document Type: Article

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