Figure 5 from The Pairing of Accreting Massive Black Holes in Multiphase Circumnuclear Disks: the Interplay Between Radiative Cooling, Star Formation, and Feedback Processes

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 5.

Vertical separation between the BHs for different runs (refer to Table 1). The plots indicate when ejections out of the disk plane occur. In the top panel (adiabatic runs), the secondary BH never exceeds the 5 pc (initial ﹩{z}_{{\rm{d}}}﹩) range from the midplane.

Other Images in This Article

Copyright and Terms & Conditions