The Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 /

The present decade is opening new frontiers in high-energy astrophysics. After the X-ray satellites in the 1980's, including Einstein, Tenma, EXOSAT and Ginga, several satellites are, or will soon be, simultaneously in orbit offering spectacular advances in X-ray imaging at low energies (ROSATj Yohkoh) as well as at high energies (GRANAT), in spectroscopy with increased bandwidth (ASCAj 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. These experiments show that the whole universe is emitting radiation at high energies, hence we call it the "hot universe. " The hot universe, preferentially emitting X- and gamma-rays, provides us with many surprises and much information. A symposium "The Hot Universe" was held in conjunction with the XXIIIrd General Assembly of the International Astronomical Union, at Kyoto on August 26-30 in 1997. The proceedings are organized as follows. Synthetic view of "the hot universe" is discussed in Section 1, "Plasma and Fresh Nucleosynthesis Phenomena". Timely discussions on the strategy for future missions "Future Space Program" are found in Section 2. Then the contents are divided into two major subjects: the compact objects and thin hot diffuse plasmas. Section 3 is devoted to the category of compact objects which includes white dwarfs, neutron stars, and gravitationally collapsed objects: stellar mass black holes or active galactic nuclei.

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Main Authors: Koyama, Katsuji. editor., Kitamoto, Shunji. editor., Itoh, Masayuki. editor., SpringerLink (Online service)
Format: Texto biblioteca
Language:eng
Published: Dordrecht : Springer Netherlands : Imprint: Springer, 1998
Subjects:Physics., Observations, Astronomical., Astronomy, Astrophysics., Astronomy, Observations and Techniques., Astrophysics and Astroparticles.,
Online Access:http://dx.doi.org/10.1007/978-94-011-4970-9
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spelling KOHA-OAI-TEST:2269662018-07-31T00:08:10ZThe Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 / Koyama, Katsuji. editor. Kitamoto, Shunji. editor. Itoh, Masayuki. editor. SpringerLink (Online service) textDordrecht : Springer Netherlands : Imprint: Springer,1998.engThe present decade is opening new frontiers in high-energy astrophysics. After the X-ray satellites in the 1980's, including Einstein, Tenma, EXOSAT and Ginga, several satellites are, or will soon be, simultaneously in orbit offering spectacular advances in X-ray imaging at low energies (ROSATj Yohkoh) as well as at high energies (GRANAT), in spectroscopy with increased bandwidth (ASCAj 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. These experiments show that the whole universe is emitting radiation at high energies, hence we call it the "hot universe. " The hot universe, preferentially emitting X- and gamma-rays, provides us with many surprises and much information. A symposium "The Hot Universe" was held in conjunction with the XXIIIrd General Assembly of the International Astronomical Union, at Kyoto on August 26-30 in 1997. The proceedings are organized as follows. Synthetic view of "the hot universe" is discussed in Section 1, "Plasma and Fresh Nucleosynthesis Phenomena". Timely discussions on the strategy for future missions "Future Space Program" are found in Section 2. Then the contents are divided into two major subjects: the compact objects and thin hot diffuse plasmas. Section 3 is devoted to the category of compact objects which includes white dwarfs, neutron stars, and gravitationally collapsed objects: stellar mass black holes or active galactic nuclei.The present decade is opening new frontiers in high-energy astrophysics. After the X-ray satellites in the 1980's, including Einstein, Tenma, EXOSAT and Ginga, several satellites are, or will soon be, simultaneously in orbit offering spectacular advances in X-ray imaging at low energies (ROSATj Yohkoh) as well as at high energies (GRANAT), in spectroscopy with increased bandwidth (ASCAj 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. These experiments show that the whole universe is emitting radiation at high energies, hence we call it the "hot universe. " The hot universe, preferentially emitting X- and gamma-rays, provides us with many surprises and much information. A symposium "The Hot Universe" was held in conjunction with the XXIIIrd General Assembly of the International Astronomical Union, at Kyoto on August 26-30 in 1997. The proceedings are organized as follows. Synthetic view of "the hot universe" is discussed in Section 1, "Plasma and Fresh Nucleosynthesis Phenomena". Timely discussions on the strategy for future missions "Future Space Program" are found in Section 2. Then the contents are divided into two major subjects: the compact objects and thin hot diffuse plasmas. Section 3 is devoted to the category of compact objects which includes white dwarfs, neutron stars, and gravitationally collapsed objects: stellar mass black holes or active galactic nuclei.Physics.Observations, Astronomical.AstronomyAstrophysics.Physics.Astronomy, Observations and Techniques.Astrophysics and Astroparticles.Springer eBookshttp://dx.doi.org/10.1007/978-94-011-4970-9URN:ISBN:9789401149709
institution COLPOS
collection Koha
country México
countrycode MX
component Bibliográfico
access En linea
En linea
databasecode cat-colpos
tag biblioteca
region America del Norte
libraryname Departamento de documentación y biblioteca de COLPOS
language eng
topic Physics.
Observations, Astronomical.
Astronomy
Astrophysics.
Physics.
Astronomy, Observations and Techniques.
Astrophysics and Astroparticles.
Physics.
Observations, Astronomical.
Astronomy
Astrophysics.
Physics.
Astronomy, Observations and Techniques.
Astrophysics and Astroparticles.
spellingShingle Physics.
Observations, Astronomical.
Astronomy
Astrophysics.
Physics.
Astronomy, Observations and Techniques.
Astrophysics and Astroparticles.
Physics.
Observations, Astronomical.
Astronomy
Astrophysics.
Physics.
Astronomy, Observations and Techniques.
Astrophysics and Astroparticles.
Koyama, Katsuji. editor.
Kitamoto, Shunji. editor.
Itoh, Masayuki. editor.
SpringerLink (Online service)
The Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 /
description The present decade is opening new frontiers in high-energy astrophysics. After the X-ray satellites in the 1980's, including Einstein, Tenma, EXOSAT and Ginga, several satellites are, or will soon be, simultaneously in orbit offering spectacular advances in X-ray imaging at low energies (ROSATj Yohkoh) as well as at high energies (GRANAT), in spectroscopy with increased bandwidth (ASCAj 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. These experiments show that the whole universe is emitting radiation at high energies, hence we call it the "hot universe. " The hot universe, preferentially emitting X- and gamma-rays, provides us with many surprises and much information. A symposium "The Hot Universe" was held in conjunction with the XXIIIrd General Assembly of the International Astronomical Union, at Kyoto on August 26-30 in 1997. The proceedings are organized as follows. Synthetic view of "the hot universe" is discussed in Section 1, "Plasma and Fresh Nucleosynthesis Phenomena". Timely discussions on the strategy for future missions "Future Space Program" are found in Section 2. Then the contents are divided into two major subjects: the compact objects and thin hot diffuse plasmas. Section 3 is devoted to the category of compact objects which includes white dwarfs, neutron stars, and gravitationally collapsed objects: stellar mass black holes or active galactic nuclei.
format Texto
topic_facet Physics.
Observations, Astronomical.
Astronomy
Astrophysics.
Physics.
Astronomy, Observations and Techniques.
Astrophysics and Astroparticles.
author Koyama, Katsuji. editor.
Kitamoto, Shunji. editor.
Itoh, Masayuki. editor.
SpringerLink (Online service)
author_facet Koyama, Katsuji. editor.
Kitamoto, Shunji. editor.
Itoh, Masayuki. editor.
SpringerLink (Online service)
author_sort Koyama, Katsuji. editor.
title The Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 /
title_short The Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 /
title_full The Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 /
title_fullStr The Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 /
title_full_unstemmed The Hot Universe [electronic resource] : Proceedings of the 188th Symposium of the International Astronomical Union Held in Kyoto, Japan, August 26–30, 1997 /
title_sort hot universe [electronic resource] : proceedings of the 188th symposium of the international astronomical union held in kyoto, japan, august 26–30, 1997 /
publisher Dordrecht : Springer Netherlands : Imprint: Springer,
publishDate 1998
url http://dx.doi.org/10.1007/978-94-011-4970-9
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