Self-Shielding of the E(1)-X(0) Band of CO in a Hot Solar Nebular

Details Self-Shielding of the E(1)-X(0) Band of CO in a Hot Solar Nebular Self-Shielding of the E(1)-X(0) Band of CO in a Hot Solar Nebular

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1999b&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1999

Physics

Scientific paper

CO self-shielding at the X-point of the early nebula has been put forth
as a possible mechanism to explain the slope-1 oxygen 3-isotope plot
observed in CAIs. We are testing this hypothesis in multiple X-point
geometries.

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