Redshift Components of Apparent Quasar-Galaxy Associations: A Parametric Model

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Quasars, Redshifts, Galaxies, Scattering

Scientific paper

The components that are known to physically contribute to an object's observed redshift are reviewed. Then, using a postulated galactic ejection model for quasars, and previously derived results from electromagnetic scattering theory which have been experimentally verified, a parametric extrapolation of these redshift components is presented. The model shows that high quasar redshift magnitudes, relative to the low redshift galaxies that eject them, can be obtained. Further, above a parametric threshold, the quasars exhibit only redshifts, despite the assumption of isotropic ejection from the galaxies. The differences in redshift between the quasars and galaxies obtained are consistent with astronomical observations of apparent physical associations. A mechanism consistent with the scattering theory and known astrophysical plasmas is suggested.

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