CO Self Shielding in the Outer Solar Nebula: An Astrochemical Explanation for the Oxygen Isotope Slope-1 Line

Details CO Self Shielding in the Outer Solar Nebula: An Astrochemical Explanation for the Oxygen Isotope Slope-1 Line CO Self Shielding in the Outer Solar Nebula: An Astrochemical Explanation for the Oxygen Isotope Slope-1 Line

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1923y&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1923

Physics

6

Scientific paper

Calculations show that photodissociation of CO by stellar EUV light high
above the midplane in the early solar nebula is an attractive and
plausible explanation for the oxygen isotope slope-1 line.

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