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Journal article

In search of live Cm-247 in the early solar system

Abstract:: The r-process only nuclide 247Cm decays to 235U with a characteristic half-life of ∼ 16 million years. 247Cm is presently extinct, but offers considerable potential as a short-lived r-process chronometer, providing constraints on the time interval between the last r-process nucleo-synthetic event and the formation of the solar system. The existence of "live" 247Cm in the early solar system should be manifested today as variations in 235U/238U, provided Cm was chemically fractionated from U wh...
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Publication status:: Published

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APA Style

Stirling, C., Halliday, A., & Porcell, D. (2005). In search of live Cm-247 in the early solar system. GEOCHIMICA ET COSMOCHIMICA ACTA, 69(4), 1059–1071.

MLA Style

Stirling, C., et al. “In Search of Live Cm-247 in the Early Solar System.” GEOCHIMICA ET COSMOCHIMICA ACTA, vol. 69, no. 4, 2005, pp. 1059–71.

Chicago Style

Stirling, C, A Halliday, and D Porcell. 2005. “In Search of Live Cm-247 in the Early Solar System.” GEOCHIMICA ET COSMOCHIMICA ACTA 69 (4): 1059–71.
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Publisher copy:: 10.1016/j.gca.2004.06.034

Authors

+ Stirling, C More by this author

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Author

+ Halliday, A More by this author

Institution:

University of Oxford

Division:

MPLS

Department:

Earth Sciences

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+ Porcell, D More by this author

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Author

Bibliographic Details

Journal:: GEOCHIMICA ET COSMOCHIMICA ACTA
Volume:: 69
Issue:: 4
Pages:: 1059-1071
Publication date:: 2005-02-15
DOI:: 10.1016/j.gca.2004.06.034
ISSN:: 0016-7037

Item Description

Language:: English
Pubs id:: pubs:82535
UUID:: uuid:3f9d88fd-f193-46b2-ac5f-f7bd5fa03b75
Local pid:: pubs:82535
Source identifiers:: 82535
Deposit date:: 2012-12-19

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Copyright date:: 2005

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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