Isotope Composition of Atomic Oxygen and Branching Ratio from CO Predissociation: Implications for Oxygen Isotope Evolution in the Early Solar Nebula

Details Isotope Composition of Atomic Oxygen and Branching Ratio from CO Predissociation: Implications for Oxygen Isotope Evolution in the Early Solar Nebula Isotope Composition of Atomic Oxygen and Branching Ratio from CO Predissociation: Implications for Oxygen Isotope Evolution in the Early Solar Nebula

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1403s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1403

Physics

Scientific paper

We investigated the "self-shielding" effects by detecting atomic ^1^6O,
^1^7O, and ^1^8O as fragments from CO predissociation. Our photonion
imaging results may help explain the different rare isotope enrichment
between N and O reported by the Genesis team.

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