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Darwin
A multi-disciplinary overview, by leading authorities, of the influence of the work of Charles Darwin on arts, science and society.
Life
An interdisciplinary exploration on the theme of 'life' with contributions from eight leading scholars across the sciences, arts and humanities.
Origins
The first book in the Darwin College Lecture series reports on the origins of the most fundamental features of our world.
Vision
Arising from the 2019 Darwin College Lectures, this book presents essays from seven prominent public intellectuals on the theme of vision. Each author examines this theme through the lens of their own particular area of expertise, making for a lively interdisciplinary volume including chapters on neuroscience, colour perception, biological evolution, astronomy, the future of technology, computer vision, and the visionary core of science. Featuring contributions by professors of neuroscience Paul Fletcher and Anya Hurlbert, professor of zoology Dan-Eric Nilsson, the futurist Sophie Hackford, Microsoft distinguished scientist Andrew Blake, theoretical physicist and author Carlo Rovelli, and Dr Carolin Crawford, the Public Astronomer at the University of Cambridge, this volume will be of interest to anybody curious about how we see the world.
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 valuable reference for research astronomers and graduate students.
Conflict
Conflict, sadly, is part of our everyday life; experienced at home, in the workplace, on our TV screens. But is it an inevitable part of the fabric of our existence? In this volume, eight experts examine conflict at many levels, from the workings of genes to the evolution of galaxies. Evolutionary biologist David Haig examines why we disagree with ourselves, and psychologist Simon Baron-Cohen asks whether differences between the average male and female mind must necessarily lead to misunderstanding. Anthropologist Richard Wrangham explores why chimpanzees and humans have evolved to kill, while archaeologist Barry Cunliffe examines the roots of warfare. Political scientist Lisa Anderson analyses conflict in the Middle East, and broadcaster Kate Adie reflects on television reporting of war. The book concludes with industrial economist William Brown's discussion of conflict in labour relations, and an exploration of the creative and destructive effects of cosmic violence by physicist P. C. W. Davies.
The X-ray Background
A review of the current observational knowledge and understanding of the cosmic X-ray background.
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 Study Institute held in Cambridge, England in July 1991. Much of the material is presented in a pedagogical manner and will appeal to scientists, astronomers and graduate students interested in extragalactic astronomy.
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 in which the gas density rises in order to maintain pressure to support the weight of the overlying gas. The rate at which mass is deposited by the flow is inferred to be several hundreds of solar masses per year in some clusters. The fraction of clust...
Physical Processes in Hot Cosmic Plasmas
Gas at temperatures exceeding one million degrees is common in the Universe. Indeed it is likely that most of the gas in the Universe exists in intergalactic space in this form. Such highly-ionized gas, or plasma, is not restricted to the rarefied densities of intergalactic space, but is also found in clusters of galaxies, in galaxies themselves, in the expanding remnants of exploded stars and at higher densities in stars and the collapsed remains of stars up to the highest densities known, which occur in neutron stars. The abundant lower-Z elements, at least, in such gas are completely ionized and the gas acts as a highly conducting plasma. It is therefore subject to many cooperative phenom...
