External UV radiation up to 10^4 G0 barely changes the inner-disk chemistry of a typical planet-forming disk, but at 10^6 G0 the disk warms, snowlines move inward, and the midplane chemistry resets to atoms and simple molecules.
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The Impact of External Radiation on the Inner Disk Chemistry of Planet Formation
External UV radiation up to 10^4 G0 barely changes the inner-disk chemistry of a typical planet-forming disk, but at 10^6 G0 the disk warms, snowlines move inward, and the midplane chemistry resets to atoms and simple molecules.