The first chemical enrichment in the universe and the formation of hyper metal-poor stars
- Author
- IWAMOTO, Nobuyuki1 ; UMEDA, Hideyuki2 ; TOMINAGA, Nozomu2 ; NOMOTO, Ken'Ichi2 ; MAEDA, Keiichi3
[1] Nuclear Data Center, Japan Atomic Energy Research Institute, Ibaraki 319-1195, Japan
[2] Department of Astronomy, School of Science, University of Tokyo, Tokyo 113-0033, Japan
[3] Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Tokyo 153-8902, Japan - Source
Science (Washington, D.C.). 2005, Vol 309, Num 5733, pp 451-453, 3 p ; ref : 28 ref
- CODEN
- SCIEAS
- ISSN
- 0036-8075
- Scientific domain
- Multidisciplinary
- Publisher
- American Association for the Advancement of Science, Washington, DC
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Abondance Effondrement Enrichissement chimique Etoile faible masse Etoile pauvre en métal Explosion supernova Modèle Mélangeage Métallicité Supernova
- Keyword (en)
- Abundance Collapse Chemical enrichment Low-mass stars Metal-poor stars Supernovae explosion Models Mixing Metallicity Supernovae
- Keyword (es)
- Desmoronamiento Enriquecimiento químico Explosión supernova Modelo Metalicidad
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C20 Normal stars (by class): general or individual / 001E03C20W Population iii stars
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16956071
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1126/science.1112997 
https://dx.doi.org/10.1126/science.1112997
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