Oxygen Isotopic Composition of Stellar Wind from the Protosun

Details Oxygen Isotopic Composition of Stellar Wind from the Protosun Oxygen Isotopic Composition of Stellar Wind from the Protosun

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1098y&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1098

Computer Science

Scientific paper

We report bimodal distribution of O isotopic composition from metal
grains in a gas-rich chondrite. The O-16-rich component seems to be
trapped solar wind of the protosun. The composition suggests no
signature of self-pollution in the solar system.

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