# Extremely Massive Quasars are not Good Proxies for Dense Environments   Compared to Massive Galaxies: Environments of Extremely Massive Quasars and   Galaxies

**Authors:** Yongmin Yoon, Myungshin Im, Minhee Hyun, Hyunsung David Jun, Narae, Hwang, Minjin Kim, and Byeong-Gon Park

arXiv: 1901.02267 · 2019-01-30

## TL;DR

Extremely massive quasars are less associated with dense environments than massive galaxies, challenging assumptions about their use as proxies for galaxy clusters and suggesting different environmental dependencies.

## Contribution

This study compares the environments of extremely massive quasars and galaxies, revealing that quasars are less often found in dense environments than massive galaxies, contrary to previous expectations.

## Key findings

- Massive quasars are in less dense environments than massive galaxies.
- Only one third of massive quasars are in galaxy clusters.
- Massive galaxies are better indicators of dense environments.

## Abstract

Black hole mass scaling relations suggest that extremely massive black holes (EMBHs) with $M_\mathrm{BH}\ge10^{9.4}\,M_{\odot}$ are found in the most massive galaxies with $M_\mathrm{star}\ge10^{11.6}\,M_{\odot}$, which are commonly found in dense environments, like galaxy clusters. Therefore, one can expect that there is a close connection between active EMBHs and dense environments. Here, we study the environments of 9461 galaxies and 2943 quasars at $0.24 \le z \le 0.40$, among which 52 are extremely massive quasars with $\log(M_\mathrm{BH}/M_{\odot}) \ge 9.4$, using Sloan Digital Sky Survey and MMT Hectospec data. We find that, on average, both massive quasars and massive galaxies reside in environments more than $\sim2$ times as dense as those of their less massive counterparts with $\log(M_\mathrm{BH}/M_{\odot}) \le 9.0$. However, massive quasars reside in environments about half as dense as inactive galaxies with $\log(M_\mathrm{BH}/M_{\odot}) \ge 9.4$, and only about one third of massive quasars are found in galaxy clusters, while about two thirds of massive galaxies reside in such clusters. This indicates that massive galaxies are a much better signpost for galaxy clusters than massive quasars. The prevalence of massive quasars in moderate to low density environments is puzzling, considering that several simulation results show that these quasars appear to prefer dense environments. Several possible reasons for this discrepancy are discussed, although further investigation is needed to obtain a definite explanation.

## Full text

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## Figures

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## References

131 references — full list in the complete paper: https://tomesphere.com/paper/1901.02267/full.md

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Source: https://tomesphere.com/paper/1901.02267