Books in the Proceedings of the International Astronomical Union Symposia and Colloquia series

Perseus provides an outstanding case study for the exploring the physics of relativistic plasma and thermal gas, and the interplay between galactic nuclei and galaxy clusters. Chapters deal with the latest results covering theory, observations, and numerical simulations, spanning a wide range in physical scales and energy ranges.

Over the past decade, modelling the panchromatic emission of galaxies has become one of the key tools in measuring their properties. IAU S341 offers a broad overview of the state of the field from theoreticians, modellers, and observers, who present and discuss the current frontier in this field.

IAU S269 celebrates the 400th anniversary of Galileo's discovery of Jupiter's largest moons. It examines our current knowledge of the Jupiter system, and considers how future space missions and instruments will improve our understanding of the potential for life in our Solar System and in the many extrasolar planetary systems.

A major goal of modern astrophysics is to understand how galaxies such as our Milky Way emerged from the primordial density fluctuations in the early Universe and how they evolved through cosmic time. IAU S352 gathers scientific contributions from theoretical and observational experts on galaxy evolution in the young Universe.

IAU Symposium 274 brings together leading experts to discuss recent observational, theoretical and experimental efforts in understanding the basic plasma processes in the Universe, from the primordial plasmas of the early Universe to stellar and laboratory plasmas. It emphasizes the importance of connecting astrophysical theory, observations, simulations and laboratory astrophysics.

IAU 282 is the product of the first official symposium to unite members of the exoplanet and binary star communities. Researchers discuss the state-of-the-art tools used to study stars, brown dwarfs and exoplanets in multiple-object systems and demonstrate how sophisticated modeling codes bridge the gap between theory and observations.

The first ever IAU Symposium to be held on the subject, reviews astronomical observations from Antarctica. Topics covered range from cosmic microwave background radiation to Antarctic stations and the future for astronomical research in Antarctica. This book is ideal for academic researchers and graduate students in astronomy and astrophysics.

A comprehensive and authoritative review of achievements in astronomy during 2010 to 2012, written by the presidents and chairpersons of the IAU scientific bodies. The reviews will appeal to colleagues in the same fields, as well as to students and researchers wanting an overview of modern astronomical research.

IAU S285 addresses studies of variability among the whole range of cosmic objects. Adopting an interdisciplinary approach, it covers both emerging transient phenomena and long-standing problems in variability. The results, research tools and visions presented here will help researchers and database managers collaborate in the exciting challenges of time-domain astronomy.

IAU S276 provides a detailed snapshot of the state-of-the-art of the field fifteen years after the first extrasolar planet discovery announcement. This volume is an important reference for scientists and researchers, who will contribute to the frontier of research in the field during the next decade.

IAU S292 provides a timely overview of galactic molecular gas and dust, and related topics including tracers of star formation and simulations of the ISM. Featuring review articles by renowned experts, and early results from the ALMA observatory, IAU S292 is perfect for graduate students and researchers in this area.

In IAU S258 astrophysicists discuss the current state of the problem of estimating ages of stars and stellar populations. They describe efforts to better constrain the ages of stars through improved observations and physical models. The volume highlights where advances are being made and predicts what the near future offers.

IAU S256 is the most complete and up-to-date account of our understanding of the Magellanic Clouds, two galaxies that accompany the Milky Way. Scientists from vastly different fields of research discuss galactic dynamics, the physics of the interstellar medium and star formation, and the fundamental properties and evolution of stars.

Archaeoastronomy and ethnoastronomy - or 'cultural astronomy' - are concerned with human practices and beliefs relating to the sky as evidenced through archaeology, history and ethnography. Through its 'building bridges' theme, this book explores the strong link between cultural astronomy and the advance of modern astronomy in the developing world.

Detailing new results and covering a broad range of topics from the origin of solar activity to the latest observational techniques, IAU Symposium 273 brings together solar and stellar astronomers to present a unified view of the field.

Galactic dynamics studies the motions of stars and gas in galaxies to understand their structure and evolution. New observations, from satellites such as Gaia, allow us to validate our theoretical models. These and other large data sets provide insights into how our Milky Way relates to the universe of galaxies.

Featuring results on the dynamical processes in stars and galaxies, IAU S271 provides a broad perspective of the observations, data analysis and theory, including numerical simulations, behind the common underlying processes in the field of nonlinear astrophysical dynamics.

IAU S260 examines the role of astronomy in the modern world and its links to culture and society. This book brings together experts and practitioners from a broad range of fields to address questions relevant to astronomy's potential contributions to education, development, culture and the arts.

IAU S272 presents an overview of the latest research into active OB stars. Experts discuss the cutting-edge observations, state-of-the-art modeling and recently developed techniques that have improved our understanding of these objects. This is a useful resource for all those interested in extreme physical processes in active OB stars.

Highlights in Astronomy summarizes the vast panorama of astronomical research at the time of the IAU's triennial General Assembly in 2012. Research by the international astronomy community is presented through a combination of extended reviews and shorter, focused chapters. This authoritative collection will appeal to research astronomers and graduate students.

IAU S310 takes a broad look at the complexity of planetary systems, including their satellites and small bodies, in order to understand and model their physical processes. Intended for researchers and advanced students, this volume provides a valuable insight into the state-of-the-art research in this exciting interdisciplinary field.

IAU Symposium 291 communicates the excitement of current pulsar research, combining lively introductory reviews with near-complete coverage of current results from across the electromagnetic spectrum. This volume is the perfect reference for neutron-star researchers and an excellent read for advanced undergraduate and graduate students.

IAU S309 presents contributions on the timely theme of spatially and energetically resolved properties of galaxies throughout cosmic history, including cutting-edge observational and computing technologies. This volume benefits astronomers and graduate students working in areas relating to galaxy formation and evolution, star formation, dust and stellar populations.

These Transactions complete the series of volumes covering the XXVII General Assembly of the International Astronomical Union. They provide a record of the admission of new members, the Resolutions passed, and an account of the regular Business Meetings of the Executive Committee, the Divisions, Commissions and Working Groups.

IAU Symposium 263 provides a state-of-the-art review of icy bodies in the Solar System, a topic that is crucial to understanding processes involved in the Solar System's formation, the consequences for water on planets, and the habitable zones around other stars.