Cool Bottom Processing on the AGB and Presolar Grain Compositions

Details Cool Bottom Processing on the AGB and Presolar Grain Compositions Cool Bottom Processing on the AGB and Presolar Grain Compositions

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1385n&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1385

Computer Science

Scientific paper

We describe results from a model of cool bottom processing in AGB stars.
We predict O, Al, C and N isotopic compositions of circumstellar grains.
Measured compositions of mainstream SiC grains and many oxide grains are
consistent with CBP.

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