Supermassive black hole fueling in IllustrisTNG: Impact of environment

Abstract

We study the association between active galactic nuclei (AGN) and environment at scales of $0.01-1h^{-1}$Mpc in the IllustrisTNG (TNG100) simulated universe. We identify supermassive black hole (BH) pairs and multiples within scales of 0.01, 0.1, & 1 $h^{-1}$Mpc and examine their AGN activity in relation to randomly-selected pairs and multiples. The number density of BHs in TNG100 is $n=0.06h^3$Mpc${}^{-3}$ at $z\lesssim 1.5$ ($n=0.02h^3$ Mpc${}^{-3}$ at $z=3$). About $\sim 10$% and $\sim 1$% of them live in pairs and multiples, respectively, within 0.1 $h^{-1}$Mpc scales. We find that BH systems have enhanced likelihood (up to factors of 3-6) of containing high Eddington ratio ($\hat{I}\cdot \gtrsim 0.7$) AGN compared to random pairs and multiples. Conversely, the likelihood of an AGN to live in 0.1$h^{-1}$Mpc scale systems is also higher (by factors $\sim 4$ for $\hat{I}\cdot \gtrsim 0.7$) compared to random pairs and multiples. We also estimate that $\sim 10$% of ultra-hard X-ray selected AGN in TNG100 have detectable 2-10 keV AGN companions on $0.1h^{-1}$Mpc scales, in agreement with observations. On larger spatial scales ($\sim 1$ $h^{-1}$Mpc), however, no significant enhancement is associated with BH pairs and multiples, even at high Eddington ratios. The enhancement of AGN activity in rich, small-scale ($\lesssim 0.1$ $h^{-1}$Mpc) environments is therefore likely to be driven by galaxy interactions and mergers. Nonetheless, the overall percentage of AGN that live in $\lesssim 0.1$ $h^{-1}$Mpc scale multiples is still subdominant (at most $\sim 40$% for the highest Eddington ratio AGN). Furthermore, the enhancement in Eddington ratios of BH systems(as well as merging BHs) is only up to factors of $\sim 2-3$. Thus, our results support the existence of a merger-AGN connection, but they also suggest that mergers and interactions play a relatively minor role in fueling the AGN population as a whole.

23 pages, 12 Figures