Bøger i Astrophysics and Space Science Library serien

The reconstruction of past solar activity is aided by studying historical accounts, which help us understand the Sun's behavior over longer timescales. Here, the authors describe how these records can be used to obtain information relevant to today's research.

Topics covered include: lessons learned and important results from earlier surveys, descriptions of some of the new surveys, clusters of galaxies and large-scale structure, radio source evolution, CMB studies, gravitational lensing and multiwavelength studies of distant radio sources.

This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such p- cesses.

As discoveries by the Dudley Observatory's astronomers, especially its second director Lewis Boss, made significant contributions to the modern vision of our Milky Way galaxy as a rotating spiral of more than a million stars, the advance of astronomy left that little observatory behind.

In late 2003 I spent two fruitful and enjoyable months in the Astronomy Department at the University of Washington (UW) working on archival material accumulated over the decades by Woody, for a book we will co-author with Jessica Chapman on the early development of Australian astronomy.

In 1988, in an article on the analysis of the measurements of the variations in the radial velocities of a number of stars, Campbell, Walker, and Yang reported an - teresting phenomenon;the radial velocity variations of Cephei seemed to suggest the existence of a Jupiter-like planet around this star.

Oftentimes, however, the supermassive black holes that lie at the centers of AGN are cocooned in gas and dust that absorb the emitted low energy X-rays and the optical and ultraviolet light, hiding the black hole from view at these wavelengths.

This book reviews the design and construction principles of radio telescopes in view of thermal aspects and heat transfer with the variable thermal environment. It is the first English language book to present and review this subject matter.

The book is written mainly to advanced graduate and post-graduate students following courses in Perturbation Theory and Celestial Mechanics. It is also intended to serve as a guide in research work and is written in a very explicit way: all perturbation theories are given with details allowing its immediate application to real problems.

This book surveys the theory of free, linear, isentropic oscillations in spherically symmetric, gaseous equilibrium stars, from basic concepts to asymptotic representations of normal modes and with slow period changes in rapidly evolving pulsating stars.

Thanks to an unprecedented resonance between X-ray, y-ray, radio and optical astronomy and important new theoretical developments in relativistic astro physics, a new deep understanding has been acquired of the physical processes oc curring in the late stages of evolution of stars.

Supernovae, hypernovae and gamma-ray bursts are among the most energetic explosions in the universe, and to understand one requires an understanding of the others. This book focuses on the similarities and differences between them. It also presents the observations that lead to these three classes of explosions.

New observations of the period between the cosmic recombination and the end of reionization are posing intriguing questions about where the first generations of stars were formed, how the first galaxies were assembled, whether these galaxies have low redshift counterparts, and what role the early galaxies played in the reionization process.

Proceedings of the XIXth ESLAB Symposium, held in Les Diablerets, Switzerland, June 4-6, 1985

Focusing on the kinetic description of the inner magnetospheric plasma, this volume illustrates how to determine the best approach to any upper atmospheric or space physics problem. Readers will find a full theoretical description of the inner magnetospheric plasma.

This book presents comprehensive coverage of the Sun and space weather, two rapidly evolving topics. In this new edition, the information has been updated to include the latest results. In addition, new sections are included, like one on space weather data sources, as well as examples and information on new satellite missions.

This book presents studies of complexity in the context of nonequilibrium phenomena using theory, modeling, simulations, and experiments, both in the laboratory and in nature.

Based on the Proceedings of the Theory Institute held at Boston College, August 9-26, 1982

Proceedings of the IAU Colloquium No. 21 held at the University of Toronto, Toronto, Canada, August 29-31, 1972

This book explores cataclysmic variables with and without strong, overpowering magnetic fields. You'll read about stars with densities ranging from that of the Sun to the degenerate matter of white dwarfs to the ultra-compact states of neutron stars and black holes.

This book explores cataclysmic variables with and without strong, overpowering magnetic fields. You'll read about stars with densities ranging from that of the Sun to the degenerate matter of white dwarfs to the ultra-compact states of neutron stars and black holes.

However, this time, thanks to the punctuality of all the participants, we have this excellent volume for the workshop on mass losing pulsating stars and their circumstellar matter prepared in time.

This book offers general information on emission line stars, starting from a brief introduction to stellar astrophysics and then moving to a broad overview of emission line stars including early and late type stars as well as pre-main sequence stars.

Based on a number of new discoveries resulting from 10 years of Chandra and XMM-Newton observations and corresponding theoretical works, this is the first book to address significant progress in the research of the Hot Interstellar Matter in Elliptical Galaxies.

This book shows the state-of-the-art in Europe on a very new discipline, Space Weather. This book reflects such a position with theoretic papers and applicative papers as well. Then, four to five contributions written by the best specialists in Europe give detailed hints of a hot topic in space weather.

This is quite simply the first volume of its kind dedicated to the area of high time resolution astrophysics. High time resolution astrophysics (HTRA) is an important new window on the universe and a vital tool in understanding a range of phenomena from diverse objects and radiative processes.

Here is a fascinating text that integrates topics pertaining to all scales of the MHD-waves, emphasizing the linkages between the ULF-waves below the ionosphere on the ground and magnetospheric MHD-waves.