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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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Covers a large range of questions, from the behaviour of dust particles to the stability of the solar system as a whole. The text also considers the motions of asteroids and their classification into families.
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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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Provides a basic introduction to kinetic plasma phenomena in solar and stellar coronae. The text explains the fundamentals of plasma physics and covers observations of coronal dynamics, such as coronal current, particle acceleration, propagation of particle beams and shocks.
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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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Aimed at active workers and graduate students in solar physics, this volume provides a comprehensive view of a rapidly expanding discipline that gives us a new perspective on the sun. Developments in infrared technology and its future are also discussed.
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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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This volume presents an up-to-date survey on investigations and results... Læs mere
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The intention of this text is to summarize the astronomical results that have affected the work of the Commission since the production of the previous reports. The reports included in the present volume range from outline summaries to lengthy compilations and references.
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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.