STRONTIUM AND BARIUM ISOTOPES IN TYPE X PRESOLAR SILICON CARBIDE GRAINS ANALYZED WITH CHILI-TWO TYPES OF SUPERNOVA GRAINS.

被引：0
作者：
Stephan, T. [1 ,2 ]
Trappitsch, R. [1 ,2 ]
Davis, A. M. [1 ,2 ,3 ]
Gyngard, F. [4 ,5 ]
Hoppe, P. [6 ]
Pellin, M. J. [1 ,2 ,3 ,7 ]
机构：
[1] Chicago Ctr Cosmochem, Chicago, IL USA
[2] Univ Chicago, Dept Geophys Sci, 5734 S Ellis Ave, Chicago, IL 60637 USA
[3] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 USA
[4] Washington Univ, Space Sci Lab, St Louis, MO USA
[5] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[6] Max Planck Inst Chem, Mainz, Germany
[7] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA
来源：
METEORITICS & PLANETARY SCIENCE | 2016年 / 51卷
关键词：
MURCHISON; NUCLEOSYNTHESIS; STARS;
D O I：
暂无
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
引用
收藏
页码：A595 / A595
页数：1
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