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Xenon, osmium, and lead formed in O-shells and C-shells of massive starsIn this paper it is shown that the explosive products from O-shells of massive stars which contain Xe-124 with large overproduction factors do not contain any of the naturally occurring isotopes of Os and Pb. Further, it is shown that the explosive products from C-shells (explosive carbon burning) do contain Os and Pb along with Xe which is strongly enriched in r-Xe of anomalous isotopic composition. The composition of Os in this matter is probably s-like rather than r-like. Pb in this matter is enriched in Pb-208. The results and arguments of this paper have implications for studies of isotopic compositions of Xe, Os, and Pb in residues of the Allende and other carbonaceous chondrites.
Document ID
19800051095
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Heymann, D.
(Rice Univ. Houston, TX, United States)
Dziczkaniec, M.
(Rice University Houston, Tex., United States)
Date Acquired
August 10, 2013
Publication Date
March 31, 1980
Publication Information
Publication: Meteoritics
Volume: 15
Subject Category
Astrophysics
Accession Number
80A35265
Funding Number(s)
CONTRACT_GRANT: NGL-44-006-127
Distribution Limits
Public
Copyright
Other

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