Figure 9 from The Pairing of Accreting Massive Black Holes in Multiphase Circumnuclear Disks: the Interplay Between Radiative Cooling, Star Formation, and Feedback Processes

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The Pairing of Accreting Massive Black Holes in Multiphase Circumnuclear Disks: the Interplay Between Radiative Cooling, Star Formation, and Feedback Processes

Authors: Rafael Souza Lima, Lucio Mayer, Pedro R. Capelo, and Jillian M. Bellovary

2017 The Astrophysical Journal 838 13.

Provider: AAS Journals

Caption: Figure 9.

Effects of the feedback mechanisms on the star formation rates in the simulations. SN feedback is the key ingredient that suppresses higher star formation rates. The introduction of AGN feedback has a negligible effect in that sense.

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