On the formation of C iii 4647-50-51 and C iii 5696 in O star atmospheres

Astronomy and Astrophysics

Volumn 545, Issue , 2012, Pages

  Martins, F ^a   Hillier, D J ^b  

^a CNRS   (France)

^b UNIVERSITY OF PITTSBURGH   (United States)

Author keywords

Stars: abundances; Stars: atmospheres; Stars: fundamental parameters; Stars: massive

Indexed keywords

ATMOSPHERE MODELS; DESATURATION; DIELECTRONIC RECOMBINATIONS; HIGH VELOCITY; LEVEL POPULATIONS; LINE PROFILES; LOW TEMPERATURES; MAIN EFFECT; MASS LOSS RATE; MASSIVE STARS; METALLIC LINES; METALLICITY EFFECT; MIXING PROCESS; OPTICAL SPECTRA; SPECTRAL TYPES; STAR ATMOSPHERES; STARS: ABUNDANCES; STARS: ATMOSPHERE; STARS: MASSIVE; STARS:FUNDAMENTAL PARAMETERS; STELLAR INTERIOR; STELLAR PARAMETERS; WIND PROPERTIES;

MODELS; OPACITY; STARS; WIND EFFECTS;

C (PROGRAMMING LANGUAGE);

EID: 84866316695     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219788     Document Type: Article

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