Surveys divide AGN into radiative-mode (accreting black holes in star-forming galaxies) and jet-mode (feedback-dominated in massive ellipticals) populations that together explain the co-evolution of galaxies and supermassive black holes.
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The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
Surveys divide AGN into radiative-mode (accreting black holes in star-forming galaxies) and jet-mode (feedback-dominated in massive ellipticals) populations that together explain the co-evolution of galaxies and supermassive black holes.