Titlebook: Introduction to Astrochemistry; Chemical Evolution f Satoshi Yamamoto Book 2017 The Editor(s) (if applicable) and The Author(s), under excl

民俗学

书目名称Introduction to Astrochemistry影响因子(影响力)




书目名称Introduction to Astrochemistry影响因子(影响力)学科排名




书目名称Introduction to Astrochemistry网络公开度




书目名称Introduction to Astrochemistry网络公开度学科排名




书目名称Introduction to Astrochemistry被引频次




书目名称Introduction to Astrochemistry被引频次学科排名




书目名称Introduction to Astrochemistry年度引用




书目名称Introduction to Astrochemistry年度引用学科排名




书目名称Introduction to Astrochemistry读者反馈




书目名称Introduction to Astrochemistry读者反馈学科排名

战役

Gratuitous

Basic Concepts for Gas-Phase Chemical Reactions,actions, dissociative electron recombination reactions, photodissociation, and photoionization are described. Timescales for chemical reactions and that for chemical equilibrium are defined in relation to rate coefficients, which are often used in the later chapters.

Urgency

Abutment

,Chemistry of Molecular Clouds II: Gas–Grain Processes, on the basis of physical processes. Depletion of molecules onto dust grains also affects chemical compositions in the gas phase. For instance, deuterium fractionation is enhanced by heavy depletion of CO. The mechanism of deuterium fractionation reactions is outlined.

GEN

Chemistry of Star-Forming Regions,le plays a crucial role in chemistry of star-forming regions. Shocks associated with outflows and accretion motions also contribute to chemical differentiation. Furthermore, photodissociation regions illuminated by young stars and nearby stars reveal unique chemistry. Key physical and chemical processes in the star-forming regions are described.

树木心

Book 2017icular emphasis on its physical and chemical background. Chemical processes in diffuse clouds, dense quiescent molecular clouds, star-forming regions, and protoplanetary disks are discussed. A brief introduction to molecular spectroscopy and observational techniques is also presented. These contents

Additive

Chemistry of Protoplanetary Disks,lined after an overview of their physical conditions. Chemical compositions are discussed for four representative parts of a disk, disk midplane, disk surface, molecular zone, and inner disk. Molecules found in comets are briefly introduced in relation to disk chemistry.

安抚

VERT

Satoshi YamamotoDraws on fundamental physics and chemistry to furnish an overview of the exotic and complex chemistry occurring in star-forming clouds.Provides a basic understanding of astrochemistry, helping readers