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Phys. Rev. Lett. 81, 3583–3586 (1998)

Strontium Isotopic Composition in Individual Circumstellar Silicon Carbide Grains: A Record of s-Process Nucleosynthesis

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G. K. Nicolussi1,2,*, M. J. Pellin2, R. S. Lewis1, A. M. Davis1,3, R. N. Clayton1,3,4, and S. Amari1,5
1Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637
2Materials Science & Chemistry Divisions, Argonne National Laboratory, Argonne, Illinois 60439
3Department of the Geophysical Sciences, University of Chicago, Chicago, Illinois 60637
4Department of Chemistry, University of Chicago, Chicago, Illinois 60637
5McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri 63130

Received 1 July 1998; published in the issue dated 26 October 1998

Twenty six individual circumstellar SiC grains extracted from the Murchison meteorite were analyzed for their strontium isotopic compositions by resonant ionization mass spectrometry. Large abundance deficits were found for the p-process isotope 84Sr. The measured grains had 87Sr/86Sr ratios indistinguishable from the primordial solar value, but several grains differed in their 88Sr/86Sr ratios as a consequence of the branch point at 85Kr. The Sr isotopic data are consistent with s-process nucleosynthesis at moderate neutron densities.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.81.3583
DOI:
10.1103/PhysRevLett.81.3583
PACS:
26.45.+h, 07.75.+h, 98.62.Bj

*Electronic address: gunther_nicolussi@qmgate.anl.gov