Continued Study of Ba Isotopic Compositions of Presolar Silicon Carbide Grains from Supernovae

Details Continued Study of Ba Isotopic Compositions of Presolar Silicon Carbide Grains from Supernovae Continued Study of Ba Isotopic Compositions of Presolar Silicon Carbide Grains from Supernovae

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1855m&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1855

Computer Science

3

Scientific paper

Ba isotopic compositions in Type X SiC grain show lower than solar
135Ba/136Ba & 137Ba/136Ba and higher than solar 138Ba/136Ba . This
can be explained by mixing of s-processed matter with
r-processed/n-burst processed matter in SN.

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