01007nam0 22002771i 450 UON0050260220231205105421.49195-11-07971-920200211d1984 |0itac50 bafinFI|||| 1||||Metsästä kaupunkiinessitä ja tutkielmia kirjallissuudestaKai LaitinenHelsingissäOtava1984333 p.22 cm.Letteratura finlandeseUONC061870FIFIHelsinkiUONL000062894.541Letteratura Finlandese21LAITINENKaiUONV153177690472OtavaUONV270694650ITSOL20251010RICASIBA - SISTEMA BIBLIOTECARIO DI ATENEOUONSIUON00502602SIBA - SISTEMA BIBLIOTECARIO DI ATENEOSI FIU A 0674 SI EO 16826 7 0674 Metsästä kaupunkiin1668694UNIOR03866nam 22007455 450 991048560500332120251113181452.03-030-75293-310.1007/978-3-030-75293-4(CKB)5590000000503263(MiAaPQ)EBC6647521(Au-PeEL)EBL6647521(OCoLC)1258220005(DE-He213)978-3-030-75293-4(PPN)269153128(EXLCZ)99559000000050326320210622d2021 u| 0engurcnu||||||||txtrdacontentcrdamediacrrdacarrierAstrophysics of the Interstellar Medium /by Giovanni Carraro1st ed. 2021.Cham :Springer International Publishing :Imprint: Springer,2021.1 online resource (361 pages)UNITEXT for Physics,2198-78903-030-75292-5 Includes bibliographical references.Fundamental 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.This 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.UNITEXT for Physics,2198-7890Soft condensed matterAcousticsElectrodynamicsPlasma confinementPlasma wavesPlasma astrophysicsFluidsAcousticsClassical ElectrodynamicsMagnetic and inertial plasma confinementWaves, instabilities and nonlinear plasma dynamicsAstrophysical PlasmaSoft condensed matter.Acoustics.Electrodynamics.Plasma confinement.Plasma waves.Plasma astrophysics.Fluids.Acoustics.Classical Electrodynamics.Magnetic and inertial plasma confinement.Waves, instabilities and nonlinear plasma dynamics.Astrophysical Plasma.523.1135Carraro Giovanni791769MiAaPQMiAaPQMiAaPQBOOK9910485605003321Astrophysics of the Interstellar Medium2045977UNINA