This text describes the gravitational interactions and evolution of astronomical systems on all scales, from small groups of stars through galaxies and clusters of galaxies to the Universe itself. In a rapidly developing area of astronomy, it is the first comprehensive treatise on the subject to be published since the early 1960s. Concentrating on the basic physics, at a graduate student level, it also develops many astronomical applications in considerable detail. The book is self-contained. Most results are derived from preceding ones in a straightforward way. It is written to bring out the physical content behind the mathematical formulae, and contains a number of exercises and suggestions for research topics. Bibliographies with nearly 300 selected references provide gateways into the literature.
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Zielgruppe
ISBN-13
978-0-511-56423-9 (9780511564239)
Schweitzer Klassifikation
Preface
Introduction
1. Idealized homogeneous systems - basic ideas and gentle relaxation
2. Infnite inhomogeneous systems - galaxy clustering
3. Finite spherical systems - cluster of galaxies, galactic nuclei, globular clusters
4. Finite flattered systems - galaxies
Index.