Chemical abundances of very metal-poor stars

Monthly Notices of the Royal Astronomical Society

Volumn 364, Issue 2, 2005, Pages 712-724

  Zhang, H W ^a,b   Zhao, G ^b  

^a PEKING UNIVERSITY   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Galaxy: halo; Stars: abundances; Stars: atmospheres; Stars: kinematics; Stars: Population II

Indexed keywords

ALUMINUM COMPOUNDS; BARIUM COMPOUNDS; CHROMIUM COMPOUNDS; COPPER COMPOUNDS; GEOMETRICAL OPTICS; IRON COMPOUNDS; KINEMATICS; MAGNESIUM COMPOUNDS; MANGANESE COMPOUNDS; METALS; NICKEL COMPOUNDS; SIGNAL TO NOISE RATIO; SILICON COMPOUNDS; SODIUM COMPOUNDS; TITANIUM COMPOUNDS; ASTROPHYSICS; GALAXIES; SODIUM IODIDE; STARS;

ELEMENT ABUNDANCES; GALAXY:HALO; METAL-POOR STAR; METALLICITIES; STARS ABUNDANCES; STARS: ATMOSPHERE; STARS: BE; STARS: KINEMATICS; STARS: POPULATION II; STELLARS;

STARS; KINEMATICS;

EID: 28744437585     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09599.x     Document Type: Article

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