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Bemærk: Kan ikke leveres før jul.
Contains a timely summary of the present knowledge of interacting binary stars. The text includes chapters covering: binary systems with compact components; the evolution of interacting binary systems; and the Algol-type interacting binaries.
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Based on the International Astronomical Union Symposium, this text covers the range of galaxies in its study of their stellar populations. Interspersed with theoretical papers, the observational results provide a presentation of the progress that has been made in the field.
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Clusters and superclusters of galaxies are the largest objects in the Universe and are... Læs mere
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Discusses in eight chapters how the conceptions of the Milky Way have moved in new directions. Starting with the inner parsec and the Centre of the Galaxy, the... Læs mere
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The motivation of the workshop and text upon which it was based was the discovery in recent years of a large number of binary and millisecond radio pulsars, in the galactic disk as well as in globular star clusters, the oldest stellar systems in the galaxy.
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Much progress has been made in understanding the internal structure of white dwarfs with asteroseismological techniques which are outlined in several papers. New observational results, which utilize this theoretical work are among the topics presented in this text.
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Containing invited essays on the bulges of spiral galaxies, this text pays detailed attention to the bulge of the Milky Way, one of the major building blocks of this system. Topics include the definition of the bulge in our galaxy and its relation to the so-called spheroid.
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Planetary nebulae are a keystone for the understanding of the evolution of stars, for deep insights into the physical processes prevailing in highly excited dilute nebulae, and for the chemical evolution in galaxies.
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Provides both the current state of observational and theoretical research, and material complementary to courses in extragalactic and interstellar astrophysics.
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The nonlinear theory of oscillating systems has introduced new aspects to the study of variable stars, allowing the appearance and disappearance of possible models to be studied in detail. This volume presents a review of the new frontiers of variable star studies.