How did the metals in a giant star originate?

被引：21

作者：

Bonifacio, P ^{[1
]}

Limongi, M

Chieffi, A

机构：

[1] Osserv Astron Trieste, Ist Nazl Astrofis, I-34131 Trieste, Italy

[2] Osserv Astron Roma, Ist Nazl Astrofis, I-00040 Rome, Italy

[3] CNR, Ist Astrofis Spaziale, I-00133 Rome, Italy

来源：

NATURE | 2003年 / 422卷 / 6934期

关键词：

D O I：

10.1038/422834a

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

[No abstract available]

引用

页码：834 / 834

页数：1

共 5 条

[1] Chemical composition of the carbon-rich, extremely metal poor star CS 29498-043: A new class of extremely metal poor stars with excesses of magnesium and silicon [J].

Aoki, W ;

Norris, JE ;

Ryan, SG ;

Beers, TC ;

Ando, H .

ASTROPHYSICAL JOURNAL, 2002, 576 (02) :L141-L144

[2] The explosive yields produced by the first generation of core collapse supernovae and the chemical composition of extremely metal poor stars [J].

Chieffi, A ;

Limongi, M .

ASTROPHYSICAL JOURNAL, 2002, 577 (01) :281-294

[3]

Chieffi A, 2002, ASTROPHYS SPACE SC L, V274, P47

[4] A stellar relic from the early Milky Way [J].

Christlieb, N ;

Bessell, MS ;

Beers, TC ;

Gustafsson, B ;

Korn, A ;

Barklem, PS ;

Karlsson, T ;

Mizuno-Wiedmer, M ;

Rossi, S .

NATURE, 2002, 419 (6910) :904-906

[5] First Stars -: II.: Elemental abundances in the extremely metal-poor star CS 22949-037 -: A diagnostic of early massive supernovae [J].

Depagne, E ;

Hill, V ;

Spite, M ;

Spite, F ;

Plez, B ;

Beers, TC ;

Barbuy, B ;

Cayrel, R ;

Andersen, J ;

Bonifacio, P ;

François, P ;

Nordström, B ;

Primas, F .

ASTRONOMY & ASTROPHYSICS, 2002, 390 (01) :187-198

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