Astronomy: The first chemical enrichment in the Universe and the formation of hyper metal-poor stars

Science

Volumn 309, Issue 5733, 2005, Pages 451-453

  Iwamoto, Nobuyuki ^a   Umeda, Hideyuki ^b   Tominaga, Nozomu ^b   Nomoto, Ken'ichi ^b   Maeda, Keiichi ^b  

^a JAPAN ATOMIC ENERGY AGENCY   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EXPLOSIONS; MATHEMATICAL MODELS; SOLAR SYSTEM;

HYPER-METAL-POOR (HMP) STARS; LOW-MASS STARS; SUPERNOVAE;

ASTROPHYSICS;

HELIUM; HYDROGEN; METAL;

SOLAR SYSTEM;

ARTICLE; ASTRONOMY; CHEMICAL COMPOSITION; COSMOS; GRAVITY; MODEL; PRIORITY JOURNAL; REPRODUCIBILITY;

EID: 22244454080     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1112997     Document Type: Article

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28. Supported by the Japan Society for the Promotion of Science and the Ministry of Education, Culture, Sports, Science, and Technology in Japan.