Abstract
The X-ray background in the energy range above 2 keV is highly uniform except for an excess component along the Galactic plane. The excess along the plane is considered to be associated with our Galaxy, whereas the rest of the emission is believed to be of extragalactic origin. In this paper, the X-ray background at high Galactic latitude is discussed and is designated as the CXB (cosmic X-ray background) to distinguish it from the Galactic origin.
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© 1998 Springer Science+Business Media Dordrecht
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Inoue, H., Takahashi, T., Ueda, Y., Yamashita, A., Ishisaki, Y., Ogasaka, Y. (1998). ASCA Sky Survey Observations and the Cosmic X-Ray Background in 2-10 Kev. In: Koyama, K., Kitamoto, S., Itoh, M. (eds) The Hot Universe. International Astronomical Union / Union Astronomique Internationale, vol 188. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4970-9_46
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DOI: https://doi.org/10.1007/978-94-011-4970-9_46
Publisher Name: Springer, Dordrecht
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