4.7 Article

CORRELATED STRONTIUM AND BARIUM ISOTOPIC COMPOSITIONS OF ACID-CLEANED SINGLE MAINSTREAM SILICON CARBIDES FROM MURCHISON

期刊

ASTROPHYSICAL JOURNAL
卷 803, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/803/1/12

关键词

circumstellar matter; meteorites, meteors, meteoroids; nuclear reactions, nucleosynthesis, abundances; stars: AGB and post-AGB; stars: carbon

资金

  1. U.S. Department of Energy, Office of Science, Materials Sciences and Engineering Division
  2. NASA Earth and Space Sciences Fellowship program [NNX11AN63H]
  3. NASA Cosmochemistry program [NNX09AG39G, NNH08AI81I]
  4. Joint Institute for Nuclear Astrophysics (JINA, University of Notre Dame, USA)
  5. Karlsruhe Institute of Technology (KIT, Karlsruhe, Germany)
  6. FIRB program [RBFR08549F-002]
  7. PRIN-MIUR Nucleosynthesis in AGB stars: An integrated approach project [20128PCN59]
  8. NASA [NNX09AG39G, 118320] Funding Source: Federal RePORTER

向作者/读者索取更多资源

We present strontium, barium, carbon, and silicon isotopic compositions of 61 acid-cleaned presolar SiC grains from Murchison. Comparison with previous data shows that acid washing is highly effective in removing both strontium and barium contamination. For the first time, by using correlated Sr-88/Sr-86 and Ba-138/Ba-136 ratios in mainstream SiC grains, we are able to resolve the effect of C-13 concentration from that of C-13-pocket mass on s-process nucleosynthesis, which points toward the existence of large C-13 pockets with low C-13 concentrations in asymptotic giant branch stars. The presence of such large C-13 pockets with a variety of relatively low C-13 concentrations seems to require multiple mixing processes in parent asymptotic giant branch stars of mainstream SiC grains.

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