Descripción del título

This book is based on a series of lectures for an Astrophysics of the Interstellar Medium (ISM) masterâs 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.
Monografía
monografia Rebiun28825032 https://catalogo.rebiun.org/rebiun/record/Rebiun28825032 DE-He213 cr nn 008mamaa 210723s2021 gw | s |||| 0|eng d 9783030752934 978-3-030-75293-4 10.1007/978-3-030-75293-4 doi UR0515950 UPVA 997742322503706 UAM 991008097611804211 UCAR 991008232112304213 CBUC 991010501211706709 UR TGM bicssc TEC021000 bisacsh TGM thema 620.11 23 Carraro, Giovanni. author. aut. http://id.loc.gov/vocabulary/relators/aut Astrophysics of the Interstellar Medium electronic resource] by Giovanni Carraro. 1st ed. 2021 Cham Springer International Publishing Imprint: Springer 2021. Cham Cham Springer International Publishing Imprint: Springer XI, 356 p. 55 illus., 16 illus. in color. online resource. XI, 356 p. 55 illus., 16 illus. in color. Text txt rdacontent computer c rdamedia online resource cr rdacarrier text file PDF rda UNITEXT for Physics 2198-7882 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) masterâs 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. Materials science. Acoustics. Optics. Electrodynamics. Plasma (Ionized gases) Materials Science, general. Acoustics. Classical Electrodynamics. Plasma Physics. SpringerLink (Online service) Springer Nature eBook Springer Nature eBook Printed edition 9783030752927 Printed edition 9783030752941 Printed edition 9783030752958 UNITEXT for Physics 2198-7882.