Supernova Remnants And Their X Ray Emission

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Supernova Remnants and their X-Ray Emission

Author : John Danziger,Paul Gorenstein
Publisher : Springer Science & Business Media
Page : 597 pages
File Size : 55,9 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400972315

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Supernova Remnants and their X-Ray Emission by John Danziger,Paul Gorenstein Pdf

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 a more unified way all of these observations. Research on supernova remnants of all ages was reported. Perhaps the most impressive part of all this work is the way in which observations at all wavelengths have extended well outside the Galaxy to other members of the Local Group and beyond. The Symposium was attended by scientists from 15 countries. Twenty five invited papers and sixty-eight shorter contributions were presented during the 4-day meeting. Thirty-three of these shorter contributions were presented in poster sessions. This volume contains almost all (89) of those contributions. They are followed by discussions which took place after each verbal presentation. Since the availability of the discussions was left to the individual contributors, they are not complete, but those contained in this volume convey some idea of the nature of the exchanges.

Supernova Remnants and Their X-ray Emission

Author : John Danziger
Publisher : Unknown
Page : 614 pages
File Size : 41,7 Mb
Release : 1983
Category : Electronic
ISBN : OCLC:252039811

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Supernova Remnants and Their X-ray Emission by John Danziger Pdf

X-ray Emission from Supernova Remnants

Author : Andrew James Sackville Hamilton
Publisher : Unknown
Page : 670 pages
File Size : 54,7 Mb
Release : 1984
Category : Supernova remnants
ISBN : UVA:X001671092

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X-ray Emission from Supernova Remnants by Andrew James Sackville Hamilton Pdf

X-ray Spectra of Supernova Remnants

Author : Andrew E. Szymkowiak
Publisher : Unknown
Page : 124 pages
File Size : 40,5 Mb
Release : 1985
Category : High Energy Astronomy Observatories
ISBN : NASA:31769000563315

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X-ray Spectra of Supernova Remnants by Andrew E. Szymkowiak Pdf

X-ray spectra were obtained from fields in three supernova remnants with the solid state spectrometer of the HEAO 2 satellite. These spectra, which contain lines from K-shell transitions of several abundant elements with atomic numbers between 10 and 22, were compared with various models, including some of spectra that would be produced by adiabatic phase remnants when the time-dependence of the ionization is considered.

An X-ray Study of Composite Supernova Remnants

Author : Jeonghee Rho
Publisher : Unknown
Page : 400 pages
File Size : 43,9 Mb
Release : 1995
Category : Supernova remnants
ISBN : UVA:X004308212

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An X-ray Study of Composite Supernova Remnants by Jeonghee Rho Pdf

Physics and Evolution of Supernova Remnants

Author : Jacco Vink
Publisher : Springer Nature
Page : 532 pages
File Size : 49,7 Mb
Release : 2020-11-10
Category : Science
ISBN : 9783030552312

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Physics and Evolution of Supernova Remnants by Jacco Vink Pdf

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 chapter is devoted to the related topic of pulsar wind nebulae, and neutron stars associated with supernova remnants. The book also includes an extended part on radiative processes, collisionless shock physics and cosmic-ray acceleration, making this book applicable to a wide variety of astronomical sub-disciplines. With its coverage of fundamental physics and careful review of the state of the field, the book serves as both textbook for advanced students and as reference for researchers in the field.

Nuclear Science Abstracts

Author : Anonim
Publisher : Unknown
Page : 810 pages
File Size : 49,9 Mb
Release : 1972
Category : Nuclear energy
ISBN : PSU:000047759480

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Nuclear Science Abstracts by Anonim Pdf

The Diversity of Neutron Stars

Author : David L. Kaplan
Publisher : Universal-Publishers
Page : 284 pages
File Size : 44,5 Mb
Release : 2004
Category : Business & Economics
ISBN : 9781581122343

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The Diversity of Neutron Stars by David L. Kaplan Pdf

Neutron stars are invaluable tools for exploring stellar death, the physics of ultra-dense matter, and the effects of extremely strong magnetic fields. The observed population of neutron stars is dominated by the >1000 radio pulsars, but there are distinct sub-populations that, while fewer in number, can have significant impact on our understanding of the issues mentioned above. These populations are the nearby, isolated neutron stars discovered by ROSAT, and the central compact objects in supernova remnants. The studies of both of these populations have been greatly accelerated in recent years through observations with the Chandra X-ray Observatory and the XMM-Newton telescope. First, we discuss radio, optical, and X-ray observations of the nearby neutron stars aimed at determining their relation to the Galactic neutron star population and at unraveling their complex physical processes by determining the basic astronomical parameters that define the population---distances, ages, and magnetic fields---the uncertainties in which limit any attempt to derive basic physical parameters for these objects. We conclude that these sources are 1e6 year-old cooling neutron stars with magnetic fields above 1e13 Gauss. Second, we describe the hollow supernova remnant problem: why many of the supernova remnants in the Galaxy have no indication of central neutron stars. We have undertaken an X-ray census of neutron stars in a volume-limited sample of Galactic supernova remnants, and from it conclude that either many supernovae do not produce neutron stars contrary to expectation, or that neutron stars can have a wide range in cooling behavior that makes many sources disappear from the X-ray sky.

Exploring the X-Ray Universe

Author : Philip A. Charles,Frederick D. Seward
Publisher : CUP Archive
Page : 420 pages
File Size : 54,7 Mb
Release : 1995-10-12
Category : Science
ISBN : 0521437121

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Exploring the X-Ray Universe by Philip A. Charles,Frederick D. Seward Pdf

The one-stop general book on the whole of X-ray astronomy.

X-Ray Astronomy

Author : R. Giacconi,H. Gursky
Publisher : Springer Science & Business Media
Page : 456 pages
File Size : 45,6 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789401021050

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X-Ray Astronomy by R. Giacconi,H. Gursky Pdf

It was about fourteen years ago that some of us became intrigued with the idea of searching the sky for X-ray and gamma-ray sources other than the Sun, the only celestial emitter of high-energy photons known at that time. It was, of course, clear that an effort in this direction would not have been successful unless there occurred, somewhere in space, processes capable of producing high-energy photons much more efficiently than the processes responsible for the radiative emission of the Sun or of ordinary stars. The possible existence of such processes became the subject of much study and discussion. As an important part of this activity, I wish to recall a one-day conference on X-ray astronomy held at the Smithsonian Astrophysical Observatory in 1960. The theoretical predictions did not provide much encouragement. While several 'unusual' celestial objects were pin-pointed as possible, or even likely, sources of X-rays, it did not look as if any of them would be strong enough to be observable with instru mentation not too far beyond the state of the art. Fortunately, we did not allow our selves to be dissuaded. As far as I am personally concerned, I must admit that my main motivation for pressing forward was a deep-seated faith in the boundless re sourcefulness of nature, which so often leaves the most daring imagination of man far behind.

Supernovae and Supernova Remnants

Author : C.B. Cosmovici
Publisher : Springer Science & Business Media
Page : 378 pages
File Size : 43,7 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789401021661

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Supernovae and Supernova Remnants by C.B. Cosmovici Pdf

This conference is a tribute to those astronomers who pioneered the investigation of this subject such a short time ago and who carried it through to its present state. (H. Arp, Concluding Remarks of the Conference) A previous conference, covering mainly the observational aspects of Supernovae, was held at the Haute Provence Observatory in September 1963. In the following ten years this field of research has considerably increased; it seemed, therefore, the right time to organize an international conference on Supernovae taking into account that in the meantime important discoveries, such as the Pulsars, had been made, and new techniques of observation were available. This book contains the proceedings of this conference held at Porto Cesareo (Lecce), Italy, during the period May 7 through 11, 1973. About one hundred participants from eighteen countries attended the conference. It was also the first attempt to hold an international conference in the Salento, the southernmost region of Apulia, in whose capital, Lecce, the newly founded Faculty of Sciences of the University of Lecce is located. The program of the conference included the results and techniques of Supernova surveys, photometric and spectral studies, statistics of Supernovae, Supernova Rem nants, and finally, theories on Supernovae and Supernova Remnants.

Neutron Stars in Supernova Remnants

Author : Patrick O. Slane,Bryan M. Gaensler
Publisher : Unknown
Page : 496 pages
File Size : 43,7 Mb
Release : 2002
Category : Science
ISBN : UOM:39015056792073

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Neutron Stars in Supernova Remnants by Patrick O. Slane,Bryan M. Gaensler Pdf

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)

High Energy Astrophysics

Author : Gerhard Börner
Publisher : Springer Science & Business Media
Page : 290 pages
File Size : 48,8 Mb
Release : 2012-12-06
Category : Science
ISBN : 9783642735608

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High Energy Astrophysics by Gerhard Börner Pdf

The second workshop on High Energy Astrophysics of the Ma..x-Planck-Society and the Academia Sinica was held at Ringberg Castle near Tegernsee during the week July 12-July 17, 1987. It is the purpose of these workshops to en courage the exchange of ideas between German and Chinese astrophysicists (scientists from other countries are also welcome, of course), and the pleas ant atmosphere and surroundings of Ringberg Castle certainly helped the development of relaxed and stimulating discussions. In addition, we seemed to have picked out the one week of perfect weather during a rainy summer. Thanks are due to Mr. Hormann and his staff for creating a perfect infra structure. The proceedings have required a considerable amount of editing, and I hope that all the papers are comprehensible. Thanks are due to Miss Petra Berkemeyer and Miss Hannelore Muller, who patiently retyped several manu scripts and helped with other editing jobs. I did not feel that a sharp refer eeing procedure should be done, although I do not agree with all the papers in this volume. The interested reader will find that this book gives a fair account of the present status of Chinese activities in the field of high energy astrophysics, i.e. in supernova physics, accretion onto compact objects, active galaxies, and cosmology.