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High Performance Computing in Science and Engineering, Garching/Munich 2009
The Leibniz Supercomputing Centre (LRZ) and the Bavarian Competence Network for Technical and Scienti?c High Performance Computing (KONWIHR) publish in the present book results of numerical simulations facilitated by the High P- formance Computer System in Bavaria (HLRB II) within the last two years. The papers were presented at the Fourth Joint HLRB and KONWIHR Review and - sult Workshop in Garching on 8th and 9th December 2009, and were selected from all progress reports of projects that use the HLRB II. Similar to the workshop two years ago, the majority of the contributed papers belong to the area of computational ?uid dynamics (CFD), condensed matter physics, astrophysics, chemistry, co...
Studying Stellar Rotation and Convection
This volume synthesizes the results of work carried out by several international teams of the SIROCO (Seismology for Rotation and Convection) collaboration. It provides the theoretical background required to interpret the huge quantity of high-quality observational data recently provided by space experiments such as CoRoT and Kepler. Asteroseismology allows astrophysicists to test, to model and to understand stellar structure and evolution as never before. The chapters in this book address the two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology". The book offers the reader solid theoretical background knowledge and adapted seismic diagnostic techniques.
The Art of Modeling Stars in the 21st Century (IAU S252)
Stellar models are the very basic building blocks with which we build up our knowledge of the Universe. New numerical experiments are heralding a new level of sophistication in our ability to model, and understand, how stars work. This volume provides an overview and the most recent advances in modeling of stellar structure and evolution. Modeling of stars relies on our understanding of the detailed physical processes happening in stars, and the most recent observations of stars made by modern large telescopes and current high technologies. IAU Symposium 252 presents the most recent developments in five key areas, including: improvements of the physical ingredients of stellar models; the evolution of low and intermediate mass stars; the evolution of massive stars; close binary evolution; and stellar physics in the era of very large telescopes. This overview of stellar research is at a level suitable for research astronomers and graduate students.
The Future of Small Telescopes in the New Millennium
This three-volume set details the essential roles that small telescopes should play in 21st century science and how their future productivity can be maximized. Over 70 international experts have created a definitive reference on the present and future of "big science with small telescopes".
Chemical Abundances in the Universe
Session I : Primordial nucleosynthesis and the first stars in the Universe -- Session II : First stars in the Galaxy -- Session III : Chemical abundances in the high red-shift Universe -- Session IV : Chemical abundance constraints on mass assembly and star formation in local galaxies and the Milky Way -- Session V : Extrasolar planets: the chemical abundance connection -- Session VI : Abundance surveys and projects in the era of future large telescopes.
Reports on Astronomy 2006-2009 (IAU XXVIIA)
The Transactions XXVIIA Reports on Astronomy 2006-2009 provides a comprehensive and authoritative review of what has been achieved in astronomy during the years 2006 to 2009. These insightful and up-to-date reviews have been written by the presidents and chairpersons of the IAU scientific bodies: the Divisions, the Commissions, and the Working Groups. Topics covered in this wide-ranging volume include: fundamental astronomy; the Sun and heliosphere; planetary sciences; stars; variable stars; interstellar matter; the Galactic system; galaxies and the Universe; optical and infrared techniques; radio astronomy; space and high-energy astrophysics; and other IAU activities. The reviews have been written at a level suitable for colleagues in the same fields, but will also be useful for students and researchers wishing to gain an overview of astronomical fields beyond their own research area.
Utopia
Utopian hope and dystopian despair are characteristic features of modernism and the avant-garde. Readings of the avant-garde have frequently sought to identify utopian moments coded in its works and activities as optimistic signs of a possible future social life, or as the attempt to preserve hope against the closure of an emergent dystopian present. The fourth volume of the EAM series, European Avant-Garde and Modernism Studies, casts light on the history, theory and actuality of the utopian and dystopian strands which run through European modernism and the avant-garde from the late 19th to the 21st century. The book’s varied and carefully selected contributions, written by experts from around 20 countries, seek to answer such questions as: · how have modernism and the avant-garde responded to historical circumstance in mapping the form of possible futures for humanity? · how have avant-garde and modernist works presented ideals of living as alternatives to the present? · how have avant-gardists acted with or against the state to remodel human life or to resist the instrumental reduction of life by administration and industrialisation?
The A-Star Puzzle (IAU S224)
Explores some of the less well understood physical processes involved in the modeling of stars.
The Evolving Sun and Its Influence on Planetary Environments
Annotation Edited by scholars from the Institute of Astrophysics of Andalusia (Spain) and Villanova U. (US), this volume contains 13 invited talks, 16 poster papers, and the introductions to three discussion sessions from the June 2001 workshop, which brought together astrophysicists, planetary physicists, and biochemists. The papers cover research into the relationship between the sun and the atmospheres, magnetospheres, and other aspects of planetary formation and characteristics. Annotation (c)2003 Book News, Inc., Portland, OR (booknews.com)
