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MARC Record from marc_columbia

Record ID marc_columbia/Columbia-extract-20221130-031.mrc:278405284:5277
Source marc_columbia
Download Link /show-records/marc_columbia/Columbia-extract-20221130-031.mrc:278405284:5277?format=raw

LEADER: 05277cam a2200721 i 4500
001 15139432
005 20220403001258.0
006 m o d
007 cr cnu|||unuuu
008 190614r20191993flua ob 001 0 eng d
035 $a(OCoLC)on1104533327
035 $a(NNC)15139432
040 $aN$T$beng$erda$epn$cN$T$dN$T$dTYFRS$dOCLCF$dUKMGB$dK6U$dOCLCO$dNLW$dOCLCQ$dOCLCO
015 $aGBB9B4765$2bnb
016 7 $a019438541$2Uk
020 $a9781315141480$q(electronic bk.)
020 $a1315141485$q(electronic bk.)
020 $a9781351454469$q(electronic bk. ;$qPDF)
020 $a1351454463$q(electronic bk. ;$qPDF)
020 $a9781351454445$q(electronic bk. ;$qMobipocket)
020 $a1351454447$q(electronic bk. ;$qMobipocket)
020 $a9781351454452$q(electronic bk. ;$qEPUB)
020 $a1351454455$q(electronic bk. ;$qEPUB)
020 $z9780750302715
024 7 $a10.1201/9781315141480$2doi
035 $a(OCoLC)1104533327
037 $a9781315141480$bTaylor & Francis
050 4 $aQB791$b.D84 2019eb
072 7 $aSCI$x004000$2bisacsh
072 7 $aSCI$x005000$2bisacsh
072 7 $aSCI$x055000$2bisacsh
072 7 $aPHVB$2bicssc
082 04 $a523/.02$223
049 $aZCUA
245 00 $aDust and chemistry in astronomy /$cedited by T.J. Millar and D.A. Williams.
264 1 $aBoca Raton, FL :$bRoutledge,$c2019.
300 $a1 online resource :$billustrations
336 $atext$btxt$2rdacontent
337 $acomputer$bc$2rdamedia
338 $aonline resource$bcr$2rdacarrier
490 1 $aThe Graduate series in astronomy
500 $aOriginally published 1993 by IOP Publishing Ltd.
504 $aIncludes bibliographical references and indexes.
588 0 $aOnline resource; title from PDF title page (EBSCO, viewed June 17, 2019).
520 $aDust is widespread in the galaxy. To astronomers studying stars it may be just an irritating fog, but it is becoming widely recognized that cosmic dust plays an active role in astrochemistry. Without dust, the galaxy would have evolved differently, and planetary systems like ours would not have occurred. To explore and consolidate this active area of research, Dust and Chemistry in Astronomy covers the role of dust in the formation of molecules in the interstellar medium, with the exception of dust in the solar system. Each chapter provides thorough coverage of our understanding of interstellar dust, particularly its interaction with interstellar gas. Aimed at postgraduate researchers, the book also serves as a thorough review of this significant area of astrophysics for practicing astronomers and graduate students.
545 0 $aT.J. Millar
505 0 $aDUST AND ASTROCHEMISTRY: AN INTRODUCTION by T.J. Millar and D.A. Williams; The Past. The Present. The Future. The Astronomical Background. Further Reading; ; OBSERVATIONS OF MOLECULAR ICES by D.C.B. Whittet; Infrared Spectroscopy. The Observed Features. Conclusions and Future Research; ; OBSERVATIONS OF HOT MOLECULAR CORES by C.M. Walmsley and P. Schilke; Observations of the Orion Hot Core. HCN Isotopomers Toward the Orion Hot Core. Observations of Other Hot Cores. Determining Physical Parameters of Hot Cores. Prospects; ; MOLECULAR HYDROGEN EMISSION FROM STAR-FORMING REGIONS by P.W.J.L. Brand; Star-Forming Regions. Shocks. Photodissociation Regions; ; CARBONACEOUS GRAINS by W.W. Duley; Bonding in Carbon Compounds. Structure of Solids. Formation of Carbon Solids. Constraints on Bonding in HAC. Electronic Transitions. Luminescence. Infrared Spectra. Comparison with Astronomical Spectra. What Is Carbonaceous Dust.
505 0 $aConclusions; ; PAHS AND ASTROCHEMISTRY by A.G.G.M. Tielens; The IR Emission Features. PAHs and C-Stardust Formation. Photochemistry of PAHs. PAHs and Ion-Molecule Chemistry. Surface Chemistry of PAHs; ; PHYSICAL AND CHEMICAL PROCESSES ON DUST by D.A. Williams; The Nature of Interstellar Dust and its Interaction with Gaseous Species. Sticking Probabilities. Mobility of Adsorbed Species. Reactions between Adsorbed Species. Ejection or Retention of Reaction Products. Mantle Processing. Desorption Processes on Interstellar Dust. Conclusion; ; INTERSTELLAR DUST AND THE CHEMISTRY OF DIFFUSE CLOUDS by R. Wagenblast and D.A. Williams; The Role of Dust in Diffuse Cloud Chemistry. HO2 (IJ) Formation on Dust. Chemical Modeling of Diffuse Clouds: Hydrides from Dust. Hydrocarbons from Shocked Dust; ; GAS-GRAIN CHEMISTRY IN QUIESCENT DENSE INTERSTELLAR CLOUDS by E. Herbst; Why Grain Chemistry Is Needed. Previous Models with Grain Reactions.
650 0 $aCosmic dust.
650 0 $aCosmochemistry.
650 6 $aPoussière cosmique.
650 6 $aCosmochimie.
650 7 $aSCIENCE$xAstronomy.$2bisacsh
650 7 $aSCIENCE$xAstrophysics & Space Science.$2bisacsh
650 7 $aSCIENCE$xPhysics.$2bisacsh
650 7 $aCosmic dust.$2fast$0(OCoLC)fst00880547
650 7 $aCosmochemistry.$2fast$0(OCoLC)fst00880582
655 4 $aElectronic books.
700 1 $aMillar, T. J.,$d1952-$eeditor.
700 1 $aWilliams, David A.,$d1937-$eeditor.
830 0 $aGraduate series in astronomy.
856 40 $uhttp://www.columbia.edu/cgi-bin/cul/resolve?clio15139432$zTaylor & Francis eBooks
852 8 $blweb$hEBOOKS