000742108 000__ 05493cam\a2200613Ii\4500 000742108 001__ 742108 000742108 005__ 20230306141229.0 000742108 006__ m\\\\\o\\d\\\\\\\\ 000742108 007__ cr\cn\nnnunnun 000742108 008__ 150911t20152016gw\a\\\\ob\\\\001\0\eng\d 000742108 019__ $$a921235858$$a931592748$$a932170763$$a932333510$$a1048170183 000742108 020__ $$a9783662478905$$q(electronic book) 000742108 020__ $$a3662478900$$q(electronic book) 000742108 020__ $$z9783662478899 000742108 020__ $$z3662478897 000742108 035__ $$aSP(OCoLC)ocn920874551 000742108 035__ $$aSP(OCoLC)920874551$$z(OCoLC)921235858$$z(OCoLC)931592748$$z(OCoLC)932170763$$z(OCoLC)932333510$$z(OCoLC)1048170183 000742108 040__ $$aN$T$$beng$$erda$$epn$$cN$T$$dGW5XE$$dN$T$$dIDEBK$$dYDXCP$$dOCLCF$$dEBLCP$$dCDX$$dOCLCA$$dOCLCQ$$dNUI$$dAZU$$dCOO$$dVT2$$dOCL$$dIOG 000742108 049__ $$aISEA 000742108 050_4 $$aQB806 000742108 08204 $$a523.8/8$$223 000742108 24500 $$aStar formation in galaxy evolution :$$bconnecting numerical models to reality : Saas-Fee Advanced course 43 /$$cSwiss Society for Astrophysics and Astronomy ; Nickolay Y. Gnedin, Simon C. O. Glover, Ralf S. Klessen, Volker Springel ; edited by Yves Revaz, Pascale Jablonka, Romain Teyssier, Lucio Mayer. 000742108 264_1 $$aHeidelberg :$$bSpringer,$$c[2015] 000742108 264_4 $$c©2016 000742108 300__ $$a1 online resource (xi, 365 pages) :$$billustrations. 000742108 336__ $$atext$$btxt$$2rdacontent 000742108 337__ $$acomputer$$bc$$2rdamedia 000742108 338__ $$aonline resource$$bcr$$2rdacarrier 000742108 4901_ $$aSaas-Fee Advanced Course,$$x1861-7980 ;$$v43 000742108 504__ $$aIncludes bibliographical references and index. 000742108 5050_ $$aPreface; Contents; Modeling Physical Processes at Galactic Scales and Above; 1 In Lieu of Introduction; 2 Physics of the IGM; 2.1 Linear Hydrodynamics in the Expanding Universe; 2.2 Lyman-α Forest; 2.3 Modeling the IGM; 2.4 What Observations Tell Us; 3 From IGM to CGM; 3.1 Large Scale Structure; 3.2 How Gas Gets onto Galaxies; 3.3 Cool Streams; 3.4 Galactic Halos; 3.5 Diversion: Cooling of Rarefied Gases; 3.6 Back to Galactic Halos; 4 ISM: Gas in Galaxies; 4.1 Galaxy Formation Lite; 4.2 Galactic Disks; 4.3 Ionized, Atomic, and Molecular Gas in Galaxies; 4.4 Molecular ISM; 5 Star Formation 000742108 5058_ $$a5.1 Kennicutt-Schmidt and All, All, All5.2 Excursion Set Formalism in Star Formation; 6 Stellar Feedback; 6.1 What Escapes from Stars; 6.2 Unconventional Marriage: Feedback and Star Formation; 6.3 Toward the Future; 7 Answers to Brain Teasers; References; Physical Processes in the Interstellar Medium; 1 Introduction; 2 Composition of the ISM; 2.1 Gas; 2.2 Dust; 2.3 Interstellar Radiation Field; 2.4 Cosmic Rays; 3 Heating and Cooling of Interstellar Gas; 3.1 Optically-Thin Two-Level Atom; 3.2 Effects of Line Opacity; 3.3 Multi-level Systems; 3.4 Atomic and Molecular Coolants in the ISM 000742108 5058_ $$a3.5 Gas-Grain Energy Transfer3.6 Computing the Dust Temperature; 3.7 Photoelectric Heating; 3.8 Other Processes Responsible for Heating; 4 ISM Turbulence; 4.1 Observations; 4.2 Simple Theoretical Considerations; 4.3 Scales of ISM Turbulence; 4.4 Decay of ISM Turbulence; 4.5 Sources of ISM Turbulence: Gravity and Rotation; 4.6 Sources of ISM Turbulence: Stellar Feedback; 5 Formation of Molecular Clouds; 5.1 Transition from Atomic to Molecular Gas; 5.2 Importance of Dust Shielding; 5.3 Molecular Cloud Formation in a Galactic Context; 6 Star Formation 000742108 5058_ $$a6.1 Molecular Cloud Cores as Sites of Star Formation6.2 Statistical Properties of Stars and Star Clusters; 6.3 Gravoturbulent Star Formation; 6.4 Theoretical Models for the Origin of the IMF; 6.5 Massive Star Formation; 6.6 Final Stages of Star and Planet Formation; 7 Summary; References; High Performance Computing and Numerical Modelling; 1 Preamble; 2 Collisionless N-Body Dynamics; 2.1 The Hierarchy of Particle Distribution Functions; 2.2 The Relaxation Time -- When Is a System Collisionless?; 2.3 N-Body Models and Gravitational Softening; 2.4 N-Body Equations in Cosmology 000742108 5058_ $$a2.5 Calculating the Dynamics of an N-Body System3 Time Integration Techniques; 3.1 Explicit and Implicit Euler Methods; 3.2 Runge-Kutta Methods; 3.3 The Leapfrog; 3.4 Symplectic Integrators; 4 Gravitational Force Calculation; 4.1 Particle Mesh Technique; 4.2 Fourier Techniques; 4.3 Multigrid Techniques; 4.4 Hierarchical Multipole Methods (``tree Codes''); 4.5 TreePM Schemes; 5 Basic Gas Dynamics; 5.1 Euler and Navier-Stokes Equations; 5.2 Shocks; 5.3 Fluid Instabilities; 5.4 Turbulence; 6 Eulerian Hydrodynamics; 6.1 Solution Schemes for PDEs; 6.2 Simple Advection; 6.3 Riemann Problem 000742108 506__ $$aAccess limited to authorized users. 000742108 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed September 17, 2015). 000742108 650_0 $$aStars$$xFormation. 000742108 650_0 $$aGalaxies$$xEvolution. 000742108 7001_ $$aGnedin, Nickolay Y.,$$d1966-$$eauthor. 000742108 7001_ $$aGlover, Simon C. O.,$$eauthor. 000742108 7001_ $$aKlessen, Ralf S.,$$eauthor. 000742108 7001_ $$aSpringel, Volker,$$eauthor. 000742108 7001_ $$aRevaz, Y.$$q(Yves),$$eeditor. 000742108 7001_ $$aJablonka, Pascale,$$eeditor. 000742108 7001_ $$aTeyssier, Romain,$$eeditor. 000742108 7001_ $$aMayer, Lucio,$$eeditor. 000742108 7102_ $$aSchweizerische Gesellschaft für Astrophysik und Astronomie,$$esponsoring body. 000742108 77608 $$iPrint version:$$z3662478897$$z9783662478899$$w(OCoLC)911210661 000742108 830_0 $$aSaas-Fee advanced course ... lecture notes ;$$v43. 000742108 85280 $$bebk$$hSpringerLink 000742108 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-662-47890-5$$zOnline Access$$91397441.1 000742108 909CO $$ooai:library.usi.edu:742108$$pGLOBAL_SET 000742108 980__ $$aEBOOK 000742108 980__ $$aBIB 000742108 982__ $$aEbook 000742108 983__ $$aOnline 000742108 994__ $$a92$$bISE