Nucleosynthetic signatures of the first stars-Reference-Cited by-同舟云学术

Nucleosynthetic signatures of the first stars

Published:2005-04 Issue:7035 Volume:434 Page:871-873
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Frebel Anna,Aoki Wako,Christlieb Norbert,Ando Hiroyasu,Asplund Martin,Barklem Paul S.,Beers Timothy C.,Eriksson Kjell,Fechner Cora,Fujimoto Masayuki Y.,Honda Satoshi,Kajino Toshitaka,Minezaki Takeo,Nomoto Ken'ichi,Norris John E.,Ryan Sean G.,Takada-Hidai Masahide,Tsangarides Stelios,Yoshii Yuzuru

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature03455.pdf

Reference30 articles.

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2. Shigeyama, T., Tsujimoto, T. & Yoshii, Y. Excavation of the first stars. Astrophys. J. 568, L57–L60 (2003)

3. Umeda, H. & Nomoto, K. First-generation black-hole-forming supernovae and the metal abundance pattern of a very iron-poor star. Nature 422, 871–873 (2003)

4. Limongi, M., Chieffi, A. & Bonifacio, P. On the origin of HE 0107–5240, the most iron-deficient star presently known. Astrophys. J. 594, L123–L126 (2003)

5. Suda, T., Aikawa, M., Machida, M. N., Fujimoto, M. Y. & Iben, I. Jr. Is HE 0107–5240 a primordial star? The characteristics of extremely metal-poor carbon-rich stars. Astrophys. J. 611, 476–493 (2004)

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