Chemistry in Protoplanetary Disks

2013/10/11 by Thomas Henning, Dmitry Semenov, Henning, Thomas +1 · 6 citations
Physics and Astronomy · #Astrophysics of Galaxies (astro-ph.GA) #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #astro-ph.EP #astro-ph.GA

paper · pdf · doi:10.48550/arxiv.1310.3151

83 pages, 8 figures, 5 tables, to be published in a Thematic Issue "Astrochemistry" in Chem. Reviews (December 2013). This document is the unedited Author's version of a Submitted Work that was subsequently accepted for publication in Chemical Reviews, copyright (c) American Chemical Society after peer review

arxiv created 2013/10/11 · arxiv updated 2013/10/14

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.

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• Intracluster ion-molecule reaction in quinoline and isoquinoline dimers under the influence of diverse ionizing radiations
• On the Efficacy of Ocean Formation with a Primordial Hydrogen Atmosphere
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