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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 7.

Circular velocity profiles centered on the primary BH’s position for runs NAC (top-left), CSF (top-right), CSFSN (bottom-left), and CSFSNBF (bottom-right). The red vertical line indicates the radial distance, projected on the disk plane, of the secondary BH from the primary one at t = 30 Myr, whereas the shaded region indicates the range of such distances during the first 30 Myr.

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