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Written by a leading expert, this monograph presents recent developments on supernova remnants, with the inclusion of results from various satellites and ground-based instruments. The book details the physics and evolution of supernova remnants, as well as provides an up-to-date account of recent multiwavelength results. Supernova remnants provide vital clues about the actual supernova explosions from X-ray spectroscopy of the supernova material, or from the imprints the progenitors had on the ambient medium supernova remnants are interacting with - all of which the author discusses in great detail. The way in which supernova remnants are classified, is reviewed and explained early on. A cha...
IAU Symposium 101, Supernova Remnants and Their X-ray Emission, was held on the Island of San Giorgio, Venice, 30 August - 2 September 1982. It was co-sponsored by the National Research Council, Italy, the University of Padua, the Observatory of Padua, and the International Astronomical Union, and was hosted by the Cini Foundation. The contents of this volume show the wide range of disciplines that are involved in supernova remnant research. Many new results were presented, not only from the X-ray observations from the Einstein Observatory but also from observations at optical and radio wavelengths. This has led to the stimulation of theoretical work, much of which attempts to accommodate in...
In the 1930s scientists discovered that the universe is expanding and that it is quite old. The observation of hydrogen lines in the spectrum of the sun helped Niels Bohr construct his atomic model in 1912, and understand the optical spectra of atoms. This era marked the transition of astronomy into astrophysics. With the rapid technological progress, scientists were able to study the universe in different ways that enabled them to observe what could not be observed using ordinary telescopes. Technology enabled scientists to see the universe in x-rays, gamma rays, radio waves and even look inside stars with neutrinos. One of the most important results of these developments, the observation o...
Proceedings of the International Conference on Supernovae, Lecce, Italy, May 7-11, 1973
A comprehensive and timely review of studies of supernovae and supernova remnants.
Annotation This book reviews both the historical observations of supernovae (SN) seen in our Galaxy over the last two millennia and recorded in East Asia (China, Japan and Korea), Europe and the Arabic dominions, together with modern observations of the remnants of these supernovae. Introductory chaptersprovide background information about the historical observations and our modern understanding of supernovae and novae, and of supernova remnants (SNRs) and pulsars. Subsequent chapters discuss the historical observations of the well defined historical SN and modern observations of their remnants. These chapters cover Kepler's SN of AD1604, Tycho's SNe of AD1572, the SN of AD1181, the SN of AD...
Annotation Slane and Gaensler (both of the Harvard-Smithsonian Center for Astrophysics) present the proceedings of an August 2001 workshop devoted to young neutron stars and their associated supernova remnants, organized in light of observational advances since a similarly themed conference in 1998. Ninety-seven papers are organized into seven sections covering rotation-powered pulsars in supernova remnants, pulsar wind theory, evolution of pulsar nebulae, observations of pulsar nebulae, exotic neutron stars and their supernova remnants, isolated and binary neutron stars, and supernovae and supernova remnants. Annotation (c)2003 Book News, Inc., Portland, OR (booknews.com)
The Crab Nebula is the single most important supernova remnant in the sky. In October 1984 several active researchers compiled this review at a workshop meeting hosted by the George Mason University. All recent theoretical and observational work is reviewed. This was no mean task because more than a decade has passed since the last international meeting on this object. New ideas covered in this volume include the Crab-like remnant in the large Magellanic Cloud; the MHD model of Crab radiation; the jet; and IUE and IRAS data. The result is an up-to-date account of the astronomy of this supernova remnant.