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Do Moderate Luminosity Active Galactic Nuclei Suppress Star Formation?

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Figure

Figure 1. Two examples of the central point-source subtraction for SDSS gr images of a morphologically disturbed galaxy (top row) and an elliptical galaxy (bottom row)
Figure 3. Timescales for “green” optical colors of AGN host galaxies. We plot three star formation scenarios probing the limits of possible color evolution based on stellar evolution models (Maraston 2005)
Figure 4. Black hole accretion rate, SFR, and optical color as a function of time, for the case of rapid (τ = 100 Myr) suppression of star formation

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