Figure 1 from The Evolution of Active Galactic Nuclei and their Spins

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The Evolution of Active Galactic Nuclei and their Spins

Authors: M. Volonteri, M. Sikora, J.-P. Lasota, and A. Merloni

Volonteri et al. 2013 The Astrophysical Journal 775 94.

Provider: AAS Journals

Caption: Figure 1.

Properties of all MBHs fed by MCs at all redshifts: normalized distribution of the masses of MBHs (top) and their host halos (bottom). The probability of MC accretion increases with galaxy mass. However, the most massive galaxies are spheroids and they therefore do not have a population of MCs available.

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