000779595 000__ 05409cam\a2200589Ii\4500
000779595 001__ 779595
000779595 005__ 20230306143027.0
000779595 006__ m\\\\\o\\d\\\\\\\\
000779595 007__ cr\nn\nnnunnun
000779595 008__ 170217s2017\\\\ja\\\\\\o\\\\\001\0\eng\d
000779595 019__ $$a973191526$$a973319660$$a973371170$$a973531835$$a973749976$$a973801480$$a973896445$$a981851163
000779595 020__ $$a9784431541714$$q(electronic book)
000779595 020__ $$a4431541713$$q(electronic book)
000779595 020__ $$z9784431541707
000779595 020__ $$z4431541705
000779595 0247_ $$a10.1007/978-4-431-54171-4$$2doi
000779595 035__ $$aSP(OCoLC)ocn972900132
000779595 035__ $$aSP(OCoLC)972900132$$z(OCoLC)973191526$$z(OCoLC)973319660$$z(OCoLC)973371170$$z(OCoLC)973531835$$z(OCoLC)973749976$$z(OCoLC)973801480$$z(OCoLC)973896445$$z(OCoLC)981851163
000779595 040__ $$aN$T$$beng$$erda$$epn$$cN$T$$dN$T$$dGW5XE$$dIDEBK$$dEBLCP$$dYDX$$dOCLCF$$dUAB$$dCOO$$dIOG$$dAZU$$dUPM
000779595 049__ $$aISEA
000779595 050_4 $$aQB450
000779595 08204 $$a523/.02$$223
000779595 1001_ $$aYamamoto, Satoshi$$c(College teacher),$$eauthor.
000779595 24510 $$aIntroduction to astrochemistry :$$bchemical evolution from interstellar clouds to star and planet formation /$$cSatoshi Yamamoto.
000779595 264_1 $$aTokyo :$$bSpringer,$$c[2017]
000779595 264_4 $$c©2017
000779595 300__ $$a1 online resource
000779595 336__ $$atext$$btxt$$2rdacontent
000779595 337__ $$acomputer$$bc$$2rdamedia
000779595 338__ $$aonline resource$$bcr$$2rdacarrier
000779595 347__ $$atext file$$bPDF$$2rda
000779595 4901_ $$aAstronomy and astrophysics library
000779595 500__ $$aIncludes index.
000779595 5050_ $$aPreface; Contents; Chapter 1: Introduction; 1.1 Matter in Space; 1.2 Interstellar Matter and Its Circulation; 1.3 Interstellar Molecules; 1.4 Importance of Chemistry; 1.5 Principal Aim of This Book; 1.6 Units Used in Astronomy; 1.7 Reaction Rates; References; Chapter 2: Derivation of Molecular Abundances; 2.1 Thermal Emission; 2.2 Information Derived from Spectral Line Observations; 2.2.1 Radiative Transfer; 2.2.2 Absorption Coefficient; 2.2.3 Optically Thin Case: Rotation Diagram Analysis; 2.2.4 Optically Thick Case; 2.3 Mechanism Determining Excitation Temperature
000779595 5058_ $$a2.4 Practical Issues for Deriving Molecular Abundances2.4.1 Source Structure; 2.4.2 Forward and Backward Approaches; 2.4.3 Molecular Parameters; References; Chapter 3: Basic Concepts for Gas-Phase Chemical Reactions; 3.1 Chemical Reactions: Macroscopic and Microscopic Viewpoints; 3.2 Reactions in Interstellar Clouds; 3.3 Ion-Molecule Reactions; 3.4 Neutral-Neutral Reactions; 3.5 Radiative Association Reactions; 3.6 Dissociative Electron Recombination; 3.7 Photodissociation and Photoionization; 3.8 Timescale of Chemical Reactions; 3.9 Timescale for Chemical Equilibrium; References
000779595 5058_ $$aChapter 4: Chemistry of Diffuse Clouds4.1 Physical Conditions in Diffuse Clouds; 4.2 Molecules Detected in Diffuse Clouds; 4.3 Carbon Chemistry; 4.4 Oxygen Chemistry; 4.5 Nitrogen Chemistry; 4.6 Chemical Model of a Diffuse Cloud; 4.7 CH+ Problem; 4.8 H3+ Problem; 4.9 Diffuse Interstellar Bands; References; Chapter 5: Chemistry of Molecular Clouds I: Gas Phase Processes; 5.1 Physical Conditions in Molecular Clouds; 5.2 Molecules in Molecular Cloud Cores; 5.3 H3+ Chemistry; 5.4 Destruction of Molecules; 5.5 Carbon Chemistry; 5.6 Oxygen Chemistry and Its Relation to Carbon Chemistry
000779595 5058_ $$a5.7 Nitrogen Chemistry5.8 Sulfur Chemistry; 5.9 Anion Chemistry; 5.10 Gas-Phase Chemical Models and Comparisons with Observations; References; Chapter 6: Chemistry of Molecular Clouds II: Gas-Grain Processes; 6.1 Roles of Dust Grains in Astrochemistry; 6.2 Depletion of Atoms and Molecules onto Dust Grains; 6.3 Grain-Surface Reactions; 6.4 Formation of H2 Molecules on Grain Surfaces; 6.5 Formation of Various Molecules on Grain Surfaces; 6.6 Desorption of Molecules by Nonthermal Processes; 6.7 Observation of Grain Mantles; 6.8 Gas-Grain Models; 6.9 Deuterium Fractionation; References
000779595 5058_ $$aChapter 7: Chemistry of Star-Forming Regions7.1 Introduction; 7.2 Formation of Low-Mass Stars; 7.3 Formation of High-Mass Stars; 7.4 Chemical Compositions of Low-Mass Star-Forming Regions; 7.4.1 Hot Corino Chemistry; 7.4.2 Warm Carbon-Chain Chemistry Sources; 7.4.3 Chemical Diversity; 7.5 Chemical Compositions of High-Mass Star-Forming Regions; 7.5.1 Orion KL; 7.5.2 W3(OH) and W3(H2O); 7.5.3 Infrared Dark Clouds; 7.6 General Features of Chemical Processes in Star-Forming Regions; 7.7 Chemical Differentiation Between Oxygen-Bearing and Nitrogen-Bearing Species
000779595 506__ $$aAccess limited to authorized users.
000779595 520__ $$aThis book draws on fundamental physics and chemistry to furnish an overview of the exotic and complex chemistry occurring in star-forming clouds. It describes chemical evolution from interstellar clouds to planetary systems.
000779595 588__ $$aOnline resource, title from PDF title page (viewed February 21, 2017).
000779595 650_0 $$aCosmochemistry.
000779595 650_0 $$aGeochemistry.
000779595 650_0 $$aMolecular evolution.
000779595 650_0 $$aLife$$xOrigin.
000779595 650_0 $$aCells$$xEvolution.
000779595 77608 $$iPrint version:$$aYamamoto, Satoshi$$tIntroduction to Astrochemistry : Chemical Evolution from Interstellar Clouds to Star and Planet Formation$$dTokyo : Springer Japan,c2017$$z9784431541707
000779595 830_0 $$aAstronomy and astrophysics library.
000779595 852__ $$bebk
000779595 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-4-431-54171-4$$zOnline Access$$91397441.1
000779595 909CO $$ooai:library.usi.edu:779595$$pGLOBAL_SET
000779595 980__ $$aEBOOK
000779595 980__ $$aBIB
000779595 982__ $$aEbook
000779595 983__ $$aOnline
000779595 994__ $$a92$$bISE