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Frontiers of X-Ray Astronomy

Fabian, A. C. (University of Cambridge) / Pounds, K. A. (University of Leicester) / Blandford, R. D. (California Institute of Technology)
Frontiers of X-Ray Astronomy
These contributions by recognized authorities originate from a Royal Society discussion meeting held to review the most recent results obtained from the current generation of X-ray telescope research. The launch of Chandra and XMM-Newton has revolutionized research in X-ray astronomy over the past few years, and high quality X-ray observations now being made have had a major impact on topics ranging from protostars to cosmology. This book is a...

CHF 115.00

Cooling Flows in Clusters and Galaxies

Fabian, A. C.
Cooling Flows in Clusters and Galaxies
X-ray astronomers discovered the diffuse gas in clusters of galaxies about 20 years ago. It was later realized that the central gas density in some clusters, and in elliptical galaxies, is so high that radiative cooling is a significant energy loss. The cooling time of the gas decreases rapidly towards the centre of the cluster or galaxy and is less than a Hubble time within the innermost few hundred kiloparsecs. This results in a cooling flow...

CHF 69.00

Clusters and Superclusters of Galaxies

Fabian, A. C.
Clusters and Superclusters of Galaxies
Clusters and superclusters of galaxies are the largest objects in the Universe. They have been the subject of intense observational studies at a variety of wavelengths, from radio to X-ray which has provoked much theoretical debate and advanced our understanding of the recent evolution of the large-scale structure of the Universe. The current status of the subject is reviewed in this volume by active researchers who lectured at a NATO Advanced...

CHF 69.00

Cooling Flows in Clusters and Galaxies

Fabian, A C
Cooling Flows in Clusters and Galaxies
X-ray astronomers discovered the diffuse gas in clusters of galaxies about 20 years ago. It was later realized that the central gas density in some clusters, and in elliptical galaxies, is so high that radiative cooling is a significant energy loss. The cooling time of the gas decreases rapidly towards the centre of the cluster or galaxy and is less than a Hubble time within the innermost few hundred kiloparsecs. This results in a cooling flow...

CHF 131.00