In chemical models of inner protoplanetary disk gas, X-ray-driven chemistry stores carbon in long-chain hydrocarbons and CO, while UV-driven chemistry stores it in atomic carbon and CO, and water strongly enhances C2H2.
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Tracking the Chemical Evolution of Hydrocarbons Through Carbon Grain Supply in Protoplanetary Disks
In chemical models of inner protoplanetary disk gas, X-ray-driven chemistry stores carbon in long-chain hydrocarbons and CO, while UV-driven chemistry stores it in atomic carbon and CO, and water strongly enhances C2H2.