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The Nature of Unidentified Galactic High-Energy Gamma-Ray Sources

The Nature of Unidentified Galactic High-Energy Gamma-Ray Sources


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About the Book

The Energetic Gamma-Ray Experiment Telescope (EGRET) instru- ment on the Compton Gamma-Ray Observatory left as a legacy its Third Catalog of High Energy Gamma-Ray Sources, whose detections include a large number of blazars, some pulsars, the Large Magellanic Cloud and a solar flare. Most of the newly discovered objects - a majority of the catalog -are unidentified sources, with a clearly predominant Galactic population. Are all these radio-quiet pulsars, like Geminga, or is there a novel type of celestial object, awaiting identification? In spite of the limited angular resolution provided by EGRET and COMPTEL, there is still much to learn about unidentified, -ray sources: correlation studies, multiwavelength observations and theoretical work can provide valuable clues, specially if these efforts are carried out in a coordinated manner. The aim of this workshop, held from October 9 to 11, 2000, at the Instituto N acional de Astrofisica, Optica y Electronica, at Tonantzintla, Mexico, was to gather experts on the subject, including observational as- tronomers specialized in other regions of the electromagnetic spectrum, in an effort to address the question of the Nature of Galactic high-energy gamma-ray sources, both from the theoretical and observational perspec- tive, and elaborate schemes for future identification studies which can make use of existing and forthcoming facilities.


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Product Details
  • ISBN-13: 9781402000102
  • Publisher: Springer
  • Publisher Imprint: Springer
  • Edition: 2001 ed.
  • Language: English
  • Returnable: N
  • Spine Width: 22 mm
  • Weight: 752 gr
  • ISBN-10: 1402000103
  • Publisher Date: 31 Oct 2001
  • Binding: Hardback
  • Height: 245 mm
  • No of Pages: 355
  • Series Title: Astrophysics and Space Science Library
  • Sub Title: Proceedings of the Workshop Held at Tonantzintla, Puebla, Mexico, 9-11 October 2000
  • Width: 158 mm


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