andrei m bykov (14 Ergebnisse)

452 p. Hardcover. Versand aus Deutschland / We dispatch from Germany via Air Mail. Einband bestoßen, daher Mängelexemplar gestempelt, sonst sehr guter Zustand. Imperfect copy due to slightly bumped cover, apart from this in very good condition. Stamped. Sprache: Englisch.

Zustand: New. In.

Zustand: New. In.

Zustand: New.

Taschenbuch. Zustand: Neu. Star Formation | Andrei M. Bykov (u. a.) | Taschenbuch | Space Sciences Series of ISSI | vi | Englisch | 2021 | Springer | EAN 9789402420647 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

547 p. Book in very good condition. 9789402417333 Sprache: Englisch Gewicht in Gramm: 1040.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The review papers in this volume provide an in-depth examination of complex astrophysical phenomena of star formation via multi-wavelength observations and modeling.Among the fundamental issues discussed in the book are:The role of gravity and magnetized turbulence in the formation and evolution of molecular cloudsThe stellar feedback (supernovae, HII regions, winds, cosmic rays) in regulating star formationThe origin of the stellar initial mass function and its universality across various environmentsJets, magnetic fields and high energy particles in stellar clustersThe origin of the first stars and black holesThe goal of these papers is to review the major processes governing star formation and to investigate how they are interlinked. In doing so, they provide an in-depth look at the tremendous theoretical and observational progress that has been made in the recent past and also outline future perspectives.Previously published inSpace Science Reviewsin the Topical Collection 'Star Formation'.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The review papers in this volume provide an in-depth examination of complex astrophysical phenomena of star formation via multi-wavelength observations and modeling.Among the fundamental issues discussed in the book are:The role of gravity and magnetized turbulence in the formation and evolution of molecular cloudsThe stellar feedback (supernovae, HII regions, winds, cosmic rays) in regulating star formationThe origin of the stellar initial mass function and its universality across various environmentsJets, magnetic fields and high energy particles in stellar clustersThe origin of the first stars and black holesThe goal of these papers is to review the major processes governing star formation and to investigate how they are interlinked. In doing so, they provide an in-depth look at the tremendous theoretical and observational progress that has been made in the recent past and also outline future perspectives.Previously published inSpace Science Reviewsin the Topical Collection 'Star Formation'.

Hardcover. Zustand: Brand New. 559 pages. 9.25x6.10x9.21 inches. In Stock.

Taschenbuch. Zustand: Neu. Clusters of Galaxies: Physics and Cosmology | Andrei M. Bykov (u. a.) | Taschenbuch | Space Sciences Series of ISSI | xii | Englisch | 2020 | Springer | EAN 9789402417364 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Clusters of galaxies are large assemblies of galaxies, hot gas and dark matter bound together by gravity. Galaxy clusters are now one of the most important cosmological probes to test the standard cosmological models. Constraints on the Dark Energy equation of state from the cluster number density measurements, deviations from the Gaussian perturbation models, the Sunyaev-Zeldovich effect as well as the dark matter proles are among the issues to be studied with clusters. The baryonic composition of clusters is dominated by hot gas that is in quasi-hydrostatic equilibrium within the dark matter-dominated gravitational potential well of the cluster. The hot gas is visible through spatially extended thermal X-ray emission, and it has been studied extensively both for assessing its physical properties and as a tracer of the large-scale structure of the Universe. Magnetic fields as well as a number of non-thermal plasma processes play a role in clusters of galaxies as we observe from radioastronomical observations.The goal of this volume is to review these processes and to investigate how they are interlinked. Overall, these papers provide a timely and comprehensive review of the multi-wavelength observations and theoretical understanding of clusters of galaxies in the cosmological context. Thus, the volume will be particularly useful to postgraduate students and researchers active in various areas of astrophysics and space science.Originally published inSpace Science Reviewsin the Topical Collection 'Clusters of Galaxies: Physics and Cosmology'.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Clusters of galaxies are large assemblies of galaxies, hot gas and dark matter bound together by gravity. Galaxy clusters are now one of the most important cosmological probes to test the standard cosmological models. Constraints on the Dark Energy equation of state from the cluster number density measurements, deviations from the Gaussian perturbation models, the Sunyaev-Zeldovich effect as well as the dark matter proles are among the issues to be studied with clusters. The baryonic composition of clusters is dominated by hot gas that is in quasi-hydrostatic equilibrium within the dark matter-dominated gravitational potential well of the cluster. The hot gas is visible through spatially extended thermal X-ray emission, and it has been studied extensively both for assessing its physical properties and as a tracer of the large-scale structure of the Universe. Magnetic fields as well as a number of non-thermal plasma processes play a role in clusters of galaxies as we observe from radioastronomical observations.The goal of this volume is to review these processes and to investigate how they are interlinked. Overall, these papers provide a timely and comprehensive review of the multi-wavelength observations and theoretical understanding of clusters of galaxies in the cosmological context. Thus, the volume will be particularly useful to postgraduate students and researchers active in various areas of astrophysics and space science.Originally published inSpace Science Reviewsin the Topical Collection 'Clusters of Galaxies: Physics and Cosmology'.

Hardcover. Zustand: Brand New. 535 pages. 9.50x6.50x1.25 inches. In Stock.

547 p. Book in very good condition. 9789402417333 Sprache: Deutsch Gewicht in Gramm: 1040.