The s-process in asymptotic giant branch (AGB) stars: Clues from zirconium and molybdenum isotopic compositions of individual presolar silicon carbide grains.

被引：0
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作者：
Nicolussi, GK
Davis, AM
Pellin, MJ
Lewis, RS
Clayton, RN
Amari, S
机构：
[1] UNIV CHICAGO,ENRICO FERMI INST,CHICAGO,IL 60637
[2] UNIV CHICAGO,DEPT GEOPHYS SCI,CHICAGO,IL 60637
[3] UNIV CHICAGO,DEPT CHEM,CHICAGO,IL 60637
[4] ARGONNE NATL LAB,DIV CHEM,ARGONNE,IL 60439
[5] ARGONNE NATL LAB,DIV MAT SCI,ARGONNE,IL 60439
[6] WASHINGTON UNIV,MCDONNELL CTR SPACE SCI,ST LOUIS,MO 63130
来源：
METEORITICS & PLANETARY SCIENCE | 1997年 / 32卷 / 04期
关键词：
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：A99 / A99
页数：1
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