research product . Lecture . 2016

The radio luminosity function and redshift evolution of radio-mode and quasar-mode AGN

Pracy, Mike;
Open Access
  • Published: 16 Aug 2016
The properties of the AGN population indicate that there are two fundamentally different accretion modes operating. In the quasar-mode, material is accreted onto the supermassive black hole via a small, thin, optically luminous accretion disc. Accretion in this mode is recognisable by emission lines in the optical spectrum. However, there is a population of AGN observable only by their radio emission and without optical emission lines. These radio-mode AGN are likely powered by radiatively inefficient accretion from a hot gas halo. I will describe the cosmic evolution of these two populations via radio luminosity functions. The radio luminosity functions are con...
arXiv: Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
free text keywords: Active Galactic Nuclei
Download from
Lecture . 2016
Provider: ZENODO
Powered by OpenAIRE Open Research Graph
Any information missing or wrong?Report an Issue