|国家预印本平台
首页|Chemistry in Protoplanetary Disks

Chemistry in Protoplanetary Disks

Chemistry in Protoplanetary Disks

来源:Arxiv_logoArxiv
英文摘要

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

天文学化学

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

评论