Buch, Englisch, Band 28, 592 Seiten, Format (B × H): 189 mm x 246 mm, Gewicht: 1136 g
Reihe: Cambridge Astrophysics
Buch, Englisch, Band 28, 592 Seiten, Format (B × H): 189 mm x 246 mm, Gewicht: 1136 g
Reihe: Cambridge Astrophysics
ISBN: 978-0-521-54209-8
Verlag: Cambridge University Press
The study of cataclysmic variables - interacting binary stars containing a white dwarf accreting from an orbiting companion - is undergoing an exciting renaissance, as it embraces observations at all wavelengths. Cataclysmic variables allow, in particular, the direct and detailed study of equilibrium and non-equilibrium accretion discs; in turn these developments also help in our understanding of X-ray binaries, black holes and active galactic nuclei. This timely volume provides the first comprehensive survey of cataclysmic variable stars, integrating theory and observation into a single, synthesised text. An introductory chapter gives the historical background of studies of cataclysmic variables. The author then goes on to give an up-to-date review of both the observations (at all wavelengths, and over all time-scales), the theories, the models of the structures and accretion processes believed to be involved. A very detailed bibliography is also provided to guide the reader to pertinent primary literature.
Autoren/Hrsg.
Fachgebiete
Weitere Infos & Material
Preface; 1. Historical development; 2. Structure of non-magnetic systems; 3. Dwarf novae; 4. Nova-like variables and nova remnants; 5. Novae in eruption; 6. Polars; 7. Intermediate polars; 8. DQ Herculis stars; 9. Evolution of cataclysmic variables; Bibliography; Index.




