Recoiling AGNs (Under Construction)

Recoiling Active Galactic Nuclei

A result of SMBH-SMBH Mergers or N-body Interactions

Details coming soon!

Explore Other System Classes

Dual AGNs

This library defines dual AGNs as having projected separations of ~0.03<rp<110 kpc .

Binary AGNs

This library defines binary AGNs as having separations of less than ~0.03 kpc (or less than ~30 pc).

N-tuple AGNs

This library includes all systems flagged as hosting or potentially hosting three or more AGNs simultaneously.