Models of α Centauri A and B with and without seismic constraints: Time dependence of the mixing-length parameter

Monthly Notices of the Royal Astronomical Society

Volumn 374, Issue 4, 2007, Pages 1264-1270

  Yildiz, M ^a  

^a EGE UNIVERSITY   (Turkey)

Author keywords

Binaries: visual; Stars: abundances; Stars: evolution; Stars: individual: Centauri; Stars: interiors; Stars: oscillations

Indexed keywords

MIXING; STARS; SYSTEMS (METALLURGICAL);

BINARIES:VISUAL; MIXING LENGTH; STAR OSCILLATIONS; STAR: EVOLUTION; STAR: INDIVIDUAL: Α CENTAURI; STARS ABUNDANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: INTERIORS; TIME DEPENDENCE; Α CEN A;

SEISMOLOGY;

EID: 33846434096     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11218.x     Document Type: Article

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