001437697 000__ 03485cam\a2200517\i\4500
001437697 001__ 1437697
001437697 003__ OCoLC
001437697 005__ 20230309004228.0
001437697 006__ m\\\\\o\\d\\\\\\\\
001437697 007__ cr\un\nnnunnun
001437697 008__ 210701s2021\\\\sz\a\\\\ob\\\\000\0\eng\d
001437697 020__ $$a9783030752934$$q(electronic bk.)
001437697 020__ $$a3030752933$$q(electronic bk.)
001437697 020__ $$z9783030752927
001437697 020__ $$z3030752925
001437697 0247_ $$a10.1007/978-3-030-75293-4$$2doi
001437697 035__ $$aSP(OCoLC)1258220005
001437697 040__ $$aYDX$$beng$$erda$$epn$$cYDX$$dGW5XE$$dEBLCP$$dOCLCO$$dOCLCF$$dUKAHL$$dOCLCQ$$dCOM$$dOCLCO$$dOCLCQ
001437697 049__ $$aISEA
001437697 050_4 $$aQB790$$b.C37 2021
001437697 08204 $$a523.1/135$$223
001437697 1001_ $$aCarraro, Giovanni,$$eauthor.
001437697 24510 $$aAstrophysics of the interstellar medium /$$cGiovanni Carraro.
001437697 264_1 $$aCham :$$bSpringer,$$c[2021]
001437697 264_4 $$c©2021
001437697 300__ $$a1 online resource :$$billustrations (some color)
001437697 336__ $$atext$$btxt$$2rdacontent
001437697 337__ $$acomputer$$bc$$2rdamedia
001437697 338__ $$aonline resource$$bcr$$2rdacarrier
001437697 4901_ $$aUNITEXT for physics,$$x2198-7882
001437697 504__ $$aIncludes bibliographical references.
001437697 5050_ $$aFundamental equations for ideal fluids -- Acoustic waves -- Real fluids -- The interstellar medium -- Shock waves -- Turbulence -- Electrodynamics and magnetohydrodynamics -- Motion of a plasma in a magnetic field -- Magnetohydrodynamic waves -- Dust from the interstellar medium -- HII regions -- Stellar Winds -- Supernovae remnants -- The interstellar medium and its components -- Molecular Clouds -- Star formation.
001437697 506__ $$aAccess limited to authorized users.
001437697 520__ $$aThis book is based on a series of lectures for an Astrophysics of the Interstellar Medium (ISM) master's degree in Astrophysics and Cosmology at Padova University. From the cold molecular phase in which stars and planetary systems form, to the very hot coronal gas that surrounds galaxies and galaxy clusters, the ISM is everywhere. Studying its properties is vital for the exploration of virtually any field in astronomy and cosmology. These notes give the student a coherent and accurate mathematical and physical approach, with continuous references to the real ISM in galaxies. The book is divided into three parts. Part One introduces the equations of fluid dynamics for a system at rest and acoustic waves, and then explores the real ISM through the role of thermal conduction and viscosity, concluding with a discussion of shock waves and turbulence. In Part Two, the electromagnetic field is switched on and its role in modulating shock waves and contrasting gravity is studied. Part Three describes dust and its properties, followed by the main stellar sources of energy. The last two chapters respectively address the various components of the ISM and molecular clouds and star formation.
001437697 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed July 6, 2021).
001437697 650_0 $$aInterstellar matter.
001437697 650_6 $$aMatière interstellaire.
001437697 655_0 $$aElectronic books.
001437697 77608 $$iPrint version:$$aCarraro, Giovanni.$$tAstrophysics of the interstellar medium.$$dCham : Springer, [2021]$$z3030752925$$z9783030752927$$w(OCoLC)1245657118
001437697 830_0 $$aUNITEXT for physics.$$x2198-7882
001437697 852__ $$bebk
001437697 85640 $$3Springer Nature$$uhttps://univsouthin.idm.oclc.org/login?url=https://link.springer.com/10.1007/978-3-030-75293-4$$zOnline Access$$91397441.1
001437697 909CO $$ooai:library.usi.edu:1437697$$pGLOBAL_SET
001437697 980__ $$aBIB
001437697 980__ $$aEBOOK
001437697 982__ $$aEbook
001437697 983__ $$aOnline
001437697 994__ $$a92$$bISE