Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-01-07
New Astron.Rev. 47 (2003) 211-214
Astronomy and Astrophysics
Astrophysics
6 pages. To appear in "Radio galaxies: past, present and future", eds M. Jarvis et al., Leiden, Nov 2002
Scientific paper
10.1016/S1387-6473(03)00027-7
Surveys to find high-redshift radio galaxies deliberately exclude optically-bright objects, which may be distant radio-loud quasars. In order to properly determine the space density of supermassive black holes, the fraction of such objects missed must be determined within a quantitative framework for AGN unification. I briefly describe the receding torus model, which predicts that quasars should have more luminous ionizing continua than radio galaxies of similar radio luminosity, and present evidence to support it. I also suggest two further tests of the model which should constrain some of its parameters.
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