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toward complete isotopic analysis of individual presolar silicon carbide grains: c, n, si, sr, zr, mo, and ba in single grains of type xThe isotopic compositions of Sr, Ba, Zr and Mo in single presolar SiC grains from supernovae are different from those expected from either of the dominant heavy element neutron capture nucleosynthesis mechanisms, the s-process and the r-process.
Document ID
20000081406
Document Type
Conference Paper
Authors
Pellin, M. J.
(Argonne National Lab. IL United States)
Calaway, W. F.
(Argonne National Lab. IL United States)
Davis, A. M.
(Chicago Univ. Chicago, IL United States)
Lewis, R. S.
(Chicago Univ. Chicago, IL United States)
Amari, S.
(Washington Univ. Saint Louis, MO United States)
Clayton, R. N.
(Chicago Univ. Chicago, IL United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Funding Number(s)
CONTRACT_GRANT: W-31-109-eng-38
CONTRACT_GRANT: NAG5-4297
CONTRACT_GRANT: NAG5-4493
CONTRACT_GRANT: NAG5-3986
CONTRACT_GRANT: NAG5-4298
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20000080557Analytic PrimaryLunar and Planetary Science XXXI