Chemistry in protoplanetary disks: analysis of uncertainties

Astronomy and Astrophysics – Astrophysics

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Modelling_Environments

Scientific paper

We identify those observable molecules in disks which modeled abundances are not greatly influenced by the uncertainties in the reaction rates of modern astrochemical networks. We demonstrate that the rate coefficients of only a handful of chemical reactions need to be determined more accurately in order to improve the reliability of disk astrochemical models.

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