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OverviewThe 1990s open new frontiers in high energy astrophysics. After the Einstein, Temma, EXOSAT and Ginga X-ray satellites of the 1980s, several satellites are simultaneously in orbit, offering spectacular advances in X-ray imaging at low energies (ROSAT; Yohkoh), as well as at high energies (GRANAT), in spectroscopy with increased bandwidth (ASCA; SAX), and in timing (XTE). While these satellites allow us to study atomic radiation from hot plasmas or energetic electrons, other satellites study nuclear radiation at gamma-ray energies (CGRO), associated with radioactivity or spallation reactions. All these experiments show that the whole universe, from the sun to clusters of galaxies, is emitting X- and gamma rays. This symposium is dedicated to highlighting high energy phenomena, in particular those seen in X- and gamma rays, and is intended to bring together the most recent results, and to discuss and deepen our insight into high energy astrophysics. Full Product DetailsAuthor: Katsuji Koyama , Shunji Kitamoto , Masayuki ItohPublisher: Springer Imprint: Springer Edition: Softcover reprint of the original 1st ed. 1998 Volume: 188 Dimensions: Width: 16.00cm , Height: 2.50cm , Length: 24.00cm Weight: 0.851kg ISBN: 9780792350590ISBN 10: 0792350596 Pages: 474 Publication Date: 31 July 1998 Audience: College/higher education , Professional and scholarly , Postgraduate, Research & Scholarly , Professional & Vocational Format: Paperback Publisher's Status: Active Availability: Out of stock ![]() The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available. Table of ContentsPreface. Session 1: Plasma and Fresh Nucleosynthesis Phenomena. 1.1. Sun and Stars. 1.2. Supernovae, Supernova Remnants and Galactic Hot Plasma. 1.3. Galaxies and Their Clusters. Session 2: Future Space Programs. Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays. 3.1. White Dwarfs and Neutron Stars. 3.2. Black Hole Binaries. 3.3. AGNs. 3.4. Gamma-Ray Bursts. Session 4: Large Scale Hot Plasmas and Their Relation with Dark Matter. Contributed Papers. Session 1: Plasma and Fresh Nucleosynthesis Phenomena. 1.1. Sun and Stars. 1.2. Supernovae, Supernova Remnants and Galactic Hot Plasma. 1.3. Galaxies and Their Clusters. Session 2: Future Space Programs. Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays. 3.1. White Dwarfs and Neutron Stars. 3.2. Black Hole Binaries. 3.3. AGNs. 3.4. Gamma-Ray Bursts. Session 4: Large Scale Hot Plasmas and Their Relation with Dark Matter.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |