Abundance analysis of Am binaries and search for tidally driven abundance anomalies - H. HD 861, HD 18778, HD 20320, HD 29479, HD 96528 and HD 108651

Monthly Notices of the Royal Astronomical Society

Volumn 370, Issue 2, 2006, Pages 819-827

  Iliev, I Kh ^a   Budaj, J ^b,c   Fenovcik M ^d   Stateva, I ^a   Richards, M T ^b  

^a National Astronomical Observatory   (Bulgaria)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c ASTRONOMICAL INSTITUTE   (Slovakia)

^d SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

Author keywords

Binaries: close; Diffusion; Hydrodynamics; Stars: abundances; Stars: chemically peculiar

Indexed keywords

GRAVITATION; STARS; VELOCITY;

ABUNDANCE ANALYSIS; BE STARS; BINARIES: CLOSE; BINARY SYSTEMS; ROTATIONAL VELOCITY; SPECTRAL REGION; STARS ABUNDANCES; STARS: CHEMICALLY PECULIAR; SYNTHETIC SPECTRA; TIDAL INTERACTIONS;

SPECTRUM ANALYSIS;

EID: 33746094244     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10513.x     Document Type: Article

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