Abundances of neutron-capture elements in G 24-25: A halo-population CH subgiant

Astronomy and Astrophysics

Volumn 541, Issue , 2012, Pages

  Liu, S ^a,b   Nissen, P E ^c   Schuster, W J ^d   Zhao, G ^a   Chen, Y Q ^a   Liang, Y C ^a  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b UNIVERSITY OF CHINESE ACADEMY OF SCIENCES   (China)

^c AARHUS UNIVERSITY   (Denmark)

^d UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: atmospheres; Stars: chemically peculiar

Indexed keywords

ABUNDANCE ANALYSIS; ABUNDANCE DISTRIBUTION; ASYMPTOTIC GIANT BRANCH; ELEMENT ABUNDANCES; EQUIVALENT WIDTH; HALO STARS; HIGH RESOLUTION; IRON GROUP; MODEL ATMOSPHERE; NUCLEAR REACTIONS , NUCLEOSYNTHESIS , ABUNDANCES; S-PROCESS; STARS: ABUNDANCES; STARS: ATMOSPHERE; STARS: CHEMICALLY PECULIAR; STELLAR PARAMETERS; WHITE DWARFS;

CARBON CAPTURE; CHEMICAL ELEMENTS; EUROPIUM; GADOLINIUM; LEAD; NEUTRONS; NUCLEOSYNTHESIS; STRONTIUM;

STARS;

EID: 84860282360     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117909     Document Type: Article

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