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X-Ray Astronomy with the Einstein Satellite: Proceedings of the High Energy Astrophysics Division of the American Astronomical Society Meeting on X-Ray Astronomy Held at the HarvardSmithsonian Center for Astrophysics, Cambridge, Massachusetts, U.S.A.

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ISBN 10: 9400984618 / ISBN 13: 9789400984615
Published by Springer
New Condition: New Soft cover
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Paperback. 330 pages. Dimensions: 9.2in. x 6.1in. x 0.8in.Riccardo Giacconi HarvardSmithsonian Center for Astrophysics The meeting of the High Energy Astrophysics Division of the American Astronomical Society, held in Cambridge, Massachusetts on January 28- 30, 1980, marks the coming of age of X-ray astronomy. In the 18 years since the discovery of the first extrasolar X-ray source, Sco X-l, the field has experienced an extremely rapid instrumentation development culminating with the launch on November 13, 1978 of the Einstein Ob servatory (HEAO-2) which first introduced the use of high resolution imaging telescopes to the study of galactic and extragalactic X-ray sources. The Einstein Observatory instruments can detect sources as faint as 10-7 Sco X-lor about 17 magnitudes fainter. The technological developments in the field have been paralleled by a host of new discoveries: in the early 1960s the detection of 9 X-ray stars, objects 10 times more luminous in X-rays than the Sun and among the brightest stellar objects at all wavelengths; in the late 1960s and early 1970s the discovery of the nature of such systems which were identified as collapsed stars (neutron stars and black holes) in mass exchange binary systems, and the detection of the first few extragalactic sources. This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN. Bookseller Inventory # 9789400984615

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Bibliographic Details

Title: X-Ray Astronomy with the Einstein Satellite:...

Publisher: Springer

Binding: Paperback

Book Condition:New

Book Type: Paperback

About this title

Synopsis:

The meeting of the High Energy Astrophysics Division of the American Astronomical Society, held in Cambridge, Massachusetts on January 28- 30, 1980, marks the coming of age of X-ray astronomy. In the 18 years since the discovery of the first extrasolar X-ray source, Sco X-l, the field has experienced an extremely rapid instrumentation development culminating with the launch on November 13, 1978 of the Einstein Observatory (HEAO-2) which first introduced the use of high resolution imaging telescopes to the study of galactic and extragalactic X-ray sources. The Einstein Observatory instruments can detect sources as faint as 10-7 Sco X-lor about 17 magnitudes fainter. The technological developments in the field have been paralleled by a host of new discoveries: in the early 1960's the detection of 9 "X-ray stars", objects 10 times more luminous in X-rays than the Sun and among the brightest stellar objects at all wavelengths; in the late 1960's and early 1970's the discovery of the nature of such systems which were identified as collapsed stars (neutron stars and black holes) in mass exchange binary systems, and the detection of the first few extragalactic sources.

About the Author:

Riccardo Giacconi, Harvard/Smithsonian Center for Astrophysics, Nobel Laureate in Physics in 2002 "for pioneering contributions to astrophysics, which have led to the discovery of cosmic X-ray sources"

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