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Laboratory astrophysics is the Rosetta Stone that enables astronomers to understand and interpret the distant cosmos. IAU S350 explores the main themes of laboratory... Læs mere
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IAU Symposium 302 provides an overview of the emerging field of stellar magnetism. Covering all stages of stellar evolution, this volume features the... Læs mere
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The physics of emission, absorption and interaction of light in astrophysics and in laboratory plasmas is developed from first principles... Læs mere
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Stars in binary and multiple systems often interact and alter the structure and evolution of the components. This volume presents state-of-the-art models... Læs mere
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Blending descriptive theoretical arguments with the latest observational results, Begelman and Rees present the evidence for black holes and their... Læs mere
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The gravitational million-body problem is a model for understanding the dynamics of rich star clusters. This... Læs mere
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The third edition of this well-established textbook is ideal for advanced undergraduate and beginning graduate courses in high energy astrophysics. Now consolidated into a... Læs mere
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Covering host systems of accreting, relativistic bodies, and the high-energy phenomena associated with them, this self-contained astrophysics textbook is ideal for... Læs mere
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Covering diverse topics from astronomy, particle physics, and cosmology, this book is ideal for researchers entering the field. Emphasizing both observational and... Læs mere
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IAU S309 presents contributions on the timely theme of spatially and energetically resolved properties of galaxies throughout cosmic history, including... Læs mere
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IAU S317 offers an updated view of the stellar halos of galaxies, from the local universe to more distant systems, discussing... Læs mere
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Aimed at graduate students and professionals, this book explores the various aspects of gamma ray burst physics, ranging from the observations on GRBs and their sources, to the theory of their creation, how they work, and how they can be used to probe the history of the Universe.