Post-processing of 3D hydrodynamic simulations with astrochemistry shows that circumplanetary gas is heated to about 800 K, releasing all volatile ices and producing sulfur-bearing molecules that may trace embedded protoplanets.
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Gas dynamics around a Jupiter mass planet: II. Chemical evolution of circumplanetary material
Post-processing of 3D hydrodynamic simulations with astrochemistry shows that circumplanetary gas is heated to about 800 K, releasing all volatile ices and producing sulfur-bearing molecules that may trace embedded protoplanets.