Quasar-illuminated dust reflection nebulae

Details Quasar-illuminated dust reflection nebulae Quasar-illuminated dust reflection nebulae

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...19710802c&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #108.02; Bulletin of the American Astronomical Society, Vol. 32, p.1585

Astronomy and Astrophysics

Astronomy

Scientific paper

The alignment effect in high redshift radio galaxies is modeled with an outward-opening, expanding, bipolar dust shell illuminated by a quasar. 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 are compared with observations of high redshift radio galaxies and quasars.

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