Chemistry in Protoplanetary Disks
Chemistry in Protoplanetary Disks
This comprehensive review summarizes our current understanding of the evolution of gas, solids and molecular ices in protoplanetary disks. Key findings related to disk physics and chemistry, both observationally and theoretically, are highlighted. We discuss which molecular probes are used to derive gas temperature, density, ionization state, kinematics, deuterium fractionation, and study organic matter in protoplanetary disks.
Dmitry Semenov、Thomas Henning
Max Planck Institute for Astronomy, HeidelbergMax Planck Institute for Astronomy, Heidelberg
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Dmitry Semenov,Thomas Henning.Chemistry in Protoplanetary Disks[EB/OL].(2013-10-11)[2025-08-02].https://arxiv.org/abs/1310.3151.点此复制
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