NASA NTRS · 19970024609
The X-ray background contributed by QSOs ejected from galaxies
Abstract
The X-ray background can be explained as coming from the integrated effect of X-ray emitting quasi-stellar objects (QSOs) ejected from spiral galaxies. The model developed to interpret the observations is summarized. The redshift of the QSOs consisted of an intrinsic component and of a cosmological component. The QSOs have a spatial density proportional to that of normal galaxies.
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Burbidge, G., Hoyle, F.. 1996-02-01. The X-ray background contributed by QSOs ejected from galaxies. https://ntrs.nasa.gov/citations/19970024609
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