Non-LTE line formation for heavy elements in four very metal-poor stars

Astronomy and Astrophysics

Volumn 478, Issue 2, 2008, Pages 529-541

  Mashonkina, L ^a,b   Zhao, G ^c   Gehren, T ^a   Aoki, W ^d   Bergemann, M ^a   Noguchi, K ^d   Shi, J R ^c   Takada Hidai, M ^e   Zhang, H W ^f  

^a UNIVERSITY OF MUNICH   (Germany)

^b INSTITUTE OF ASTRONOMY   (Russian Federation)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^e TOKAI UNIVERSITY   (Japan)

^f PEKING UNIVERSITY   (China)

Author keywords

Line: formation; Line: profiles; Stars: abundances; Stars: fundamental parameters; Stars: general; Stars: late type

Indexed keywords

LINE: FORMATION; LINE: PROFILES; STARS: ABUNDANCES; STARS: FUNDAMENTAL PARAMETERS; STARS: GENERAL; STARS: LATE-TYPE;

BARIUM; CALCIUM; EUROPIUM; GEOMETRICAL OPTICS; IONIZATION; ISOTOPES; RESONANCE; SODIUM; SOLAR SYSTEM; STRONTIUM; TEMPERATURE;

STARS;

EID: 43949097937     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078060     Document Type: Article

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