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OverviewGalaxies have a history. This has become clear from sky surveys, which have shown that distant galaxies, formed early in the life of the Universe, differ from the nearby ones. Observational windows at ultraviolet, infrared and millimetric wavelengths (provided by ROSAT, IRAM, IUE, IRAS, ISO) have revealed that galaxies contain a wealth of components: very hot gas, atomic hydrogen, molecules, dust, and dark matter. Three Euroconferences planned to punctuate advances in galactic research, brought together specialists in various fields of astronomy. The first, held in Granada, Spain in May 2000, addressed the observational clues. The second took place in October 2001 in St Denis de la Reunion, France) and reviewed the basic building blocks and small-scale processes in galaxy evolution. The third is scheduled to take place in July 2002 in Kiel, Germany and will be devoted to the overall modelling of galaxy evolution. This book contains the proceedings of the second conference. Full Product DetailsAuthor: Marc Sauvage , Grazyna Stasinska , D. SchaererPublisher: Springer-Verlag New York Inc. Imprint: Springer-Verlag New York Inc. Edition: 2002 ed. Dimensions: Width: 15.50cm , Height: 3.10cm , Length: 23.50cm Weight: 2.160kg ISBN: 9781402006227ISBN 10: 1402006225 Pages: 562 Publication Date: 31 July 2002 Audience: College/higher education , Professional and scholarly , Postgraduate, Research & Scholarly , Professional & Vocational Format: Hardback Publisher's Status: Active Availability: In Print ![]() This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us. Table of ContentsIntroductory Session.- 1: Star Formation.- 2: Nucleosynthesis and Stellar Evolution.- 3: Energy Flows in the Interstellar Medium.- 4: Environmental Effects on Galaxy Evolution.- 5: Primeval Stars and Galaxies.- List of Participants.- Author Index.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |