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Author: William Butler Burton
Publisher: Springer Science & Business Media
ISBN: 9789027710307
Category : Juvenile Nonfiction
Languages : en
Pages : 638
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Book Description
At head of title: International Astronomical Union. Union astronomique internationale.
Author: William Butler Burton
Publisher: Springer Science & Business Media
ISBN: 9789027710307
Category : Juvenile Nonfiction
Languages : en
Pages : 638
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Book Description
At head of title: International Astronomical Union. Union astronomique internationale.
Author: William Butler Burton
Publisher: Springer
ISBN:
Category : Science
Languages : en
Pages : 644
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Book Description
Proceedings of IAU Symposium No. 84 held at College Park, Maryland, U.S.A., June 12-17, 1978
Author: Lars E. B. Johansson
Publisher:
ISBN:
Category :
Languages : en
Pages : 64
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Book Description
Author: Jan P Mucket
Publisher: World Scientific
ISBN: 9814548936
Category :
Languages : en
Pages : 394
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Book Description
This volume documents the theoretical and observational results and arguments in favour of (or against) the most preferred models of structure formation. New observational results of the large scale distribution of matter are confronted with recent theories on the origin and evolution of structure in the universe.
Author: William Butler Burton
Publisher: Springer
ISBN: 9789027710307
Category : Science
Languages : en
Pages : 61
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Book Description
Author: Hugo van Woerden
Publisher: Springer Science & Business Media
ISBN: 9400952910
Category : Science
Languages : en
Pages : 684
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Book Description
In June 1983 the Astronomical Institute of the State University of Groningen, founded by Kapteyn about 100 years ago, celebrated its one-hundredth anniversary. At the suggestion of its Chairman, R.J. Allen, the Kapteyn Institute invited the International Astronomical Union to mark the centenary by holding a Symposium on "The Milky Way Galaxy". The purpose of the Symposium was to review recent progress in the study of our Galaxy, to define current problems, and to explore prospects for future development. The Symposium programme would emphasize the large-scale characteristics of our Galaxy, and highlight both the historical development of our understanding of the Milky Way Galaxy and the importance of studies of external galaxies to this understanding. The Symposium was sponsored by four IAU Commissions: 33 (Structure and Dynamics of the Galactic System), 28 (Galaxies), 34 (Interstellar Matter) and 41 (History of Astronomy). The Scientific Organizing Committee, listed on page xviii, represented a broad range of nationalities and of expertise, including two historians of science. A meeting of the Committee, held during the IAU General Assembly at Patras, provided an excellent opportunity to discuss plan and format of the Symposium, topics and speakers; thereafter, the-Committee was regularly consulted by letter and telephone. IAU Symposium 106 was held at Groningen on 30 May - 3 June 1983, in the new building occupied by the Kapteyn Institute since January 1983. There were about 200 participants, coming from as many as 25 countries.
Author: Manolis Plionis
Publisher: Springer
ISBN: 1402069413
Category : Science
Languages : en
Pages : 476
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Book Description
The reviews presented in this volume cover a huge range of cluster of galaxies topics. Readers will find the book essential reading on subjects such as the physics of the ICM gas, the internal cluster dynamics, and the detection of clusters using different observational techniques. The expert chapter authors also cover the huge advances being made in analytical or numerical modeling of clusters, weak and strong lensing effects, and the large scale structure as traced by clusters.
Author: Lars E. B. Johansson
Publisher:
ISBN:
Category :
Languages : en
Pages : 64
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Book Description
Author: National Radio Astronomy Observatory (U.S.)
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 492
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Book Description
Author: A.A. Ruzmaikin
Publisher: Springer Science & Business Media
ISBN: 9400928351
Category : Science
Languages : en
Pages : 322
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Book Description
Magnetism, when extended beyond normal frameworks into cosmic space is characterized by an enormous spatial scale. Because of their large sizes the nature of magnets such as the Earth and the Sun is entirely different from the nature of a horseshoe magnet. The source of cosmic magnetism is associated with the hydrodynamic motions of a highly conductive medium. In this aspect, cosmic magnets resemble a dynamo. However, currents in the dynamo flow along properly ordered wires, while chaotic, turbulent motions are dominant inside stars and liquid planetary cores. This makes more intriguing and surprising the fact that these motions maintain a regular magnetic field. Maintenance of magnetic fields is even more impressive in huge magnets, i.e. galaxies. In fact, we are living inside a giant dynamo machine, the Milky Way galaxy. Although the idea of the global magnetic field of our Galaxy was clearly proposed almost 40 years ago, firm observational evidence and definite theoretical concepts of galactic magnetism have been developed only in the last decade. This book is the first attempt at a full and consistent presentation of this problem. We discuss both theoretical views on the origin of galactic magnetism and the methods of observational study. Previous discussions were on the level of review articles or separate chapters in monographs devoted to cosmic magnetic fields (see, e.g., H. K. Moffatt, 1978, E. N. Parker, 1979 and Zeldovich et aI., 1983).
