Chemistry in Protoplanetary Disks
by Thomas Henning, Dmitry Semenov
Publisher: arXiv 2013
Number of pages: 84
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.
Home page url
Download or read it online for free here:
by M. De Becker - arXiv
Astrochemistry aims at studying chemical processes in astronomical environments. This discipline is rapidly evolving and explores the issue of the formation of molecules of increasing complexity in particular physical conditions...
by F. Aharonian, A. Bykov, E. Parizot, V. Ptuskin, A. Watson - arXiv
We review sources of cosmic rays, their composition and spectra as well as their propagation in the galactic and extragalactic magnetic fields, both regular and fluctuating. A special attention is paid to the recent results of the observations.
by Jonathan P. Williams, Lucas A. Cieza - arXiv
Flattened disks of cool dust and gas are found around almost all low mass stars shortly after their birth. This review addresses observations of the outer parts of protoplanetary disks with a focus on recent infrared and (sub-)millimeter results.
- Rice University
This 1400+ pages book covers the very rapidly growing area of star-and-planet formation and evolution, from astrophysics to planetary science. It is most useful for researchers, graduate students, and some undergraduate students.