LEADER 01610nam a2200301 i 4500 001 991000579949707536 008 050901s2000 enka b 001 0 eng d 020 $a0471959022 035 $ab13879017-39ule_inst 040 $aDip.to Ingegneria dell'Innovazione$beng 082 0 $a541.3$221 084 $aLC QD453.3 100 1 $aKuhn, Hans,$d1919-$0472554 245 10$aPrinciples of physical chemistry :$bunderstanding molecules, molecular assemblies, supramolecular machines /$cHans Kuhn and Horst-Dieter Försterling 260 $aChichester ;$aNew York :$bWiley,$cc2000 300 $axxviii, 970 p. :$bill. ;$c26 cm 504 $aIncludes bibliographical references and index 650 4$aChemistry, Physical and theoretical 700 1 $aFörsterling, Horst-Dieter$eauthor$4http://id.loc.gov/vocabulary/relators/aut$0606036 856 4 $zTable of Contents$uhttp://www.loc.gov/catdir/toc/onix02/98048542.html 907 $a.b13879017$b07-04-22$c05-02-10 912 $a991000579949707536 945 $aLE026 541.3 D KUH 01.01 C.1 2000$cC.1$g1$i2026000054780$lle026$nProf. Valli / Biblioteca$op$pE75.03$q-$rn$s- $t1$u0$v0$w0$x0$y.i1507092x$z08-02-10 945 $aLE026 541.3 D KUH 01.01 C.2 2000$cC.2$g1$i2026000054797$lle026$nProf. Valli / Biblioteca$op$pE75.03$q-$rn$so $t4$u1$v0$w1$x0$y.i15070931$z08-02-10 945 $aLE006 Fondo Polezzo 275$cEx libris Stefano Polezzo$g1$i2006000181884$lle006$og$pE48.82$q-$rl$s- $t0$u0$v0$w0$x0$y.i15947130$z14-01-21 996 $aPrinciples of physical chemistry$91440655 997 $aUNISALENTO 998 $ale026$ale006$b11-05-20$cm$da $e-$feng$genk$h0$i0 LEADER 04973nam 22007215 450 001 9910254572203321 005 20200703041122.0 010 $a3-662-54350-8 024 7 $a10.1007/978-3-662-54350-4 035 $a(CKB)3710000001152002 035 $a(DE-He213)978-3-662-54350-4 035 $a(MiAaPQ)EBC4838373 035 $z(PPN)258847905 035 $a(PPN)200510061 035 $a(EXLCZ)993710000001152002 100 $a20170408d2017 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 12$aA Dirty Window $eDiffuse and Translucent Molecular Gas in the Interstellar Medium /$fby Loris Magnani, Steven N. Shore 205 $a1st ed. 2017. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d2017. 215 $a1 online resource (XIX, 306 p. 76 illus., 28 illus. in color.) 225 1 $aAstrophysics and Space Science Library,$x0067-0057 ;$v442 311 $a3-662-54348-6 320 $aIncludes bibliographical references at the end of each chapters and index. 327 $aA quick look at the diffuse interstellar medium -- Radiative transfer considerations -- The diffuse ISM from the ground - chemistry and tracers -- Observing the diffuse ISM - making sense of the radio observations -- Observing the diffuse ISM - the space missions -- Observing in the Dark: The Dust-Gas Connection -- Surveying the molecular Milky Way -- The relationship between CO and H2 -- Surveys for high-latitude molecular clouds -- Distances -- Dynamical Considerations: Instabilities and Turbulence -- Coda.-. 330 $aThis book provides an introduction to the physics of interstellar gas in the Galaxy. It deals with the diffuse interstellar medium which supplies a complex environment for exploring the neutral gas content of a galaxy like the Milky Way and the techniques necessary for studying this non-stellar component. After an initial exposition of the phases of the interstellar medium and the role of gas in a spiral galaxy, the authors discuss the transition from atomic to molecular gas. They then consider basic radiative transfer and molecular spectroscopy with particular emphasis on the molecules useful for studying low-density molecular gas. Observational techniques for investigating the gas and the dust component of the diffuse interstellar medium throughout the electromagnetic spectrum are explored emphasizing results from the recent Herschel and Planck missions. A brief exposition on dust in the diffuse interstellar medium is followed by a discussion of molecular clouds in general and high-latitude molecular clouds in particular. Ways of calibrating CO observations with the molecular hydrogen content of a cloud are examined along with the dark molecular gas controversy. High-latitude molecular clouds are considered in detail as vehicles for applying the techniques developed in the book. Given the transient nature of diffuse and translucent molecular clouds, the role of turbulence in the origin and dynamics of these objects is examined in some detail. The book is targeted at graduate students or postdocs who are entering the field of interstellar medium studies. 410 0$aAstrophysics and Space Science Library,$x0067-0057 ;$v442 606 $aAstrophysics 606 $aAstronomy$vObservations 606 $aAstronomy?Observations 606 $aExobiology 606 $aSpace sciences 606 $aCosmology 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aAstrobiology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22057 606 $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030 606 $aCosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22049 615 0$aAstrophysics. 615 0$aAstronomy 615 0$aAstronomy?Observations. 615 0$aExobiology. 615 0$aSpace sciences. 615 0$aCosmology. 615 14$aAstrophysics and Astroparticles. 615 24$aAstronomy, Observations and Techniques. 615 24$aAstrobiology. 615 24$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 615 24$aCosmology. 676 $a523.0196 700 $aMagnani$b Loris$4aut$4http://id.loc.gov/vocabulary/relators/aut$0892438 702 $aShore$b Steven N$4aut$4http://id.loc.gov/vocabulary/relators/aut 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910254572203321 996 $aA Dirty Window$91993181 997 $aUNINA