Meteoritic Stardust and the Clumpiness of Galactic Chemical Evolution

Details Meteoritic Stardust and the Clumpiness of Galactic Chemical Evolution Meteoritic Stardust and the Clumpiness of Galactic Chemical Evolution

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1650n&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1650

Physics

2

Scientific paper

We discuss a model of heterogeneous galactic chemical evolution.
Although the model can explain presolar SiC Si isotopes, it fails to
predict correlations between Si and Ti isotopes or the observed range of
O isotopes in presolar oxide grains.

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