pith. sign in

arxiv: 1310.3151 · v1 · pith:6PIBU3GOnew · submitted 2013-10-11 · 🌌 astro-ph.GA · astro-ph.EP

Chemistry in Protoplanetary Disks

classification 🌌 astro-ph.GA astro-ph.EP
keywords disksprotoplanetarychemistrymolecularcomprehensivecurrentdensityderive
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. From Young to Older Disks: JWST/MIRI Evidence for Fading Molecular Emission and Hints for Elevated C/O in Upper Scorpius

    astro-ph.EP 2026-06 unverdicted novelty 7.0

    Older Upper Scorpius disks show reduced molecular emission and hints of higher inner-gas C/O ratios than young disks, indicating chemical evolution consistent with pebble drift.