Polarimetry of the aligned optical continuua in high redshift radio galaxies

Details Polarimetry of the aligned optical continuua in high redshift radio galaxies Polarimetry of the aligned optical continuua in high redshift radio galaxies

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.4504c&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #45.04; Bulletin of the American Astronomical Society, Vol. 34, p.714

Astronomy and Astrophysics

Astronomy

Scientific paper

Replace these paragraphs with your abstract. We encourage you to include a sentence acknowledging your funding agency. Milky Way and SMC dust grain models are used to model the quasar-illuminated dust reflection nebulae that contribute to the alignment effect in high redshift radio galaxies. The model explains why QSRs have little or no extinction while allowing for the alignment effect in HZRGs to be dominated by dust scattering and still preserving the unification of radio galaxies and quasars. Model images, spectra, and polarization images will be compared with observations of high redshift radio galaxies and quasars.

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