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The diffuse soft X-ray sky

Astrophysics related to cosmic soft X-rays in the energy range 0.1–2.0 keV

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Abstract

The current status of the investigation of the soft X-ray diffuse background in the energy range 0.1–2.0 keV is reviewed. A consistent model, based on the soft X-ray brightness distribution and the energy spectrum over the sky, is derived. The observed diffuse background is predominantly of galactic origin and considered as thermal emission for the most part from a local hot region of temperature ≈106 K which includes the solar system. Several pronounced features of enhanced emission are interpreted in terms of hot regions with temperatures up to 3×106K, some of which are probably old supernova remnants. The properties of the soft X-ray emitting regions are discussed in relation to the observational results on O vi absorption.

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  1. Institute of Space and Aeronautical Science, University of Tokyo, Tokyo, Japan

    Y. Tanaka

  2. Huygens Laboratory, University of Leiden, Leiden, the Netherlands

    J. A. M. Bleeker

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Tanaka, Y., Bleeker, J.A.M. The diffuse soft X-ray sky. Space Sci Rev 20, 815–888 (1977). https://doi.org/10.1007/BF02431836

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