The X-ray background contributed by QSOs ejected from galaxies.

Details The X-ray background contributed by QSOs ejected from galaxies. The X-ray background contributed by QSOs ejected from galaxies.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..307b&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 307 - 310

Astronomy and Astrophysics

Astrophysics

X-Ray Background: Quasars

Scientific paper

It is shown that the X-ray background radiation can be explained as coming from the integrated effect of X-ray emitting quasi-stellar objects which have been ejected from spiral galaxies. In this model the redshift of the QSOs are made up of two components, an intrinsic component zi, and a cosmological component zc, such that the observed redshift zobs is given by (1+zobs) = (1+zi)(1+zc). In this model the QSOs have a density in space proportional to that of normal galaxies, so that no evolution is required. The typical values of zc are ≡0.1 to 0.2.

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