High-resolution optical spectroscopy of the sharp-lined B-type star HD 83206

Monthly Notices of the Royal Astronomical Society

Volumn 314, Issue 1, 2000, Pages 199-208

  Lehner, N ^a   Dufton, P L ^a   Lambert, D L ^b   Ryans, R S I ^a   Keenan, F P ^a  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b The University of Texas at Austin   (United States)

Author keywords

Stars: abundances; Stars: atmospheres; Stars: early type; Stars: individual: HD 83206

Indexed keywords

METALS; STARS;

ATMOSPHERIC PARAMETERS; METAL ABUNDANCES; METAL LINE; MODEL ATMOSPHERE; NON-LTE; STAR: INDIVIDUAL: HD 83206; STARS ABUNDANCES; STARS: ATMOSPHERE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:EARLY TYPE;

SILICON COMPOUNDS;

EID: 0041491306     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03294.x     Document Type: Article

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