Modelling the components of binaries in the Hyades: The dependence of the mixing-length parameter on stellar mass

Monthly Notices of the Royal Astronomical Society

Volumn 368, Issue 4, 2006, Pages 1941-1948

  Yildiz, M ^a   Yakut, K ^a,b   Bakis H ^c   Noels, A ^d  

^a EGE UNIVERSITY   (Turkey)

^b UNIVERSITY OF LEUVEN   (Belgium)

^c ÇANAKKALE ONSEKIZ MART UNIVERSITY   (Turkey)

^d UNIVERSITY OF LIÈGE   (Belgium)

Author keywords

Binaries: eclipsing; Open clusters and associations: individual: Hyades; Stars: abundances; Stars: evolution; Stars: interiors

Indexed keywords

MIXING; SPECTROSCOPIC ANALYSIS; STARS;

BINARIES:ECLIPSING; BINARY SYSTEMS; CHEMICAL COMPOSITIONS; FITTING FORMULA; MIXING LENGTH; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: HYADES; STAR: EVOLUTION; STARS ABUNDANCES; STARS: INTERIORS; STELLAR MASS;

SYSTEMS (METALLURGICAL);

EID: 33744550598     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10275.x     Document Type: Article

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