Abundance analysis of Am binaries and search for tidally driven abundance anomalies -I. HD 33254, HD 178449 and HD 198391

Monthly Notices of the Royal Astronomical Society

Volumn 346, Issue 1, 2003, Pages 27-36

  Budaj, J ^a,b   Iliev, I Kh ^c  

^a ASTRONOMICAL INSTITUTE   (Slovakia)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c National Astronomical Observatory   (Bulgaria)

Author keywords

Binaries: close; Diffusion; Stars: chemically peculiar; Stars: individual: HD 178449; Stars: individual: HD 198391; Stars: individual: HD 33254

Indexed keywords

CHEMICAL ANALYSIS; SPECTRUM ANALYSIS;

ABUNDANCE ANALYSIS; BINARIES: CLOSE; MERIDIONAL CIRCULATION; STAR: INDIVIDUAL: HD 178449; STAR: INDIVIDUAL: HD 198391; STAR: INDIVIDUAL: HD 33254; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI;

STARS;

EID: 0344493941     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-2966.2003.07071.x     Document Type: Article

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