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タイトルDiffuse Gamma Rays Galactic and Extragalactic Diffuse Emission
本文(外部サイト)http://hdl.handle.net/2060/20040037787
著者(英)Strong, Andrew W.; Moskalenko, Igor V.; Reimer, Olaf
著者所属(英)NASA Goddard Space Flight Center
発行日2004-01-01
言語eng
内容記述Diffuse gamma rays consist of several components: truly diffuse emission from the interstellar medium, the extragalactic background, whose origin is not firmly established yet, and the contribution from unresolved and faint Galactic point sources. One approach to unravel these components is to study the diffuse emission from the interstellar medium, which traces the interactions of high energy particles with interstellar gas and radiation fields. Because of its origin such emission is potentially able to reveal much about the sources and propagation of cosmic rays. The extragalactic background, if reliably determined, can be used in cosmological and blazar studies. Studying the derived average spectrum of faint Galactic sources may be able to give a clue to the nature of the emitting objects.
NASA分類Astronomy
権利Copyright, Distribution as joint owner in the copyright


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