Plasma Redshift in the Broad Line Region [PDF]
Peter M. HansenAstronomical properties of the broad line emission region (BLR) of active galactic nuclei (AGN) and quasi-stellar objects (QSO) are used to formulate a model of dynamic and electromagnetic scattering characteristics. The results of this modeling show that the observed redshift of these objects may be more complex than that from recession alone due to ionization or plasma effects.View original: http://arxiv.org/abs/1301.1705
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