Evaluating CO Self-Shielding and the Oxygen Isotopic Evolution of the Solar Protoplanetary Disk with Astrochemical Reaction Networks

Details Evaluating CO Self-Shielding and the Oxygen Isotopic Evolution of the Solar Protoplanetary Disk with Astrochemical Reaction Networks Evaluating CO Self-Shielding and the Oxygen Isotopic Evolution of the Solar Protoplanetary Disk with Astrochemical Reaction Networks

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1790y&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1790

Physics

2

Scientific paper

A quantitative model for the oxygen isotopic evolution of the early
solar system is presented. The model is based on combining a detailed
reaction network with mass transport among reservoirs in the
protoplanetary disk.

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