Turbulent Mixing Chemistry in Disks

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

A gas-grain chemical model with surface reaction and 1D/2D turbulent mixing is available for protoplanetary disks and molecular clouds. Current version is based on the updated UMIST'95 database with gas-grain interactions (accretion, desorption, photoevaporation, etc.) and modified rate equation approach to surface chemistry (see also abstract for the static chemistry code).

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