Chemistry in Protoplanetary Disks
by Thomas Henning, Dmitry Semenov
Publisher: arXiv 2013
Number of pages: 84
Description:
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.
Download or read it online for free here:
Download link
(2.1MB, PDF)
Similar books
Astrochemistry: The Issue of Molecular Complexity in Astrophysical Environmentsby 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...
(7695 views)
Protoplanetary Disks and Their Evolutionby 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.
(10181 views)
Protostars and Planets- 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.
(16654 views)
An Introduction to Galactic Chemical Evolutionby Nikos Prantzos - arXiv
The formalism of the simple model of galactic chemical evolution (GCE) and its main ingredients are presented. It is stressed that GCE is not an astrophysical theory, but it provides a framework in which the large body of data may be interpreted.
(10031 views)