Effect of bars in AGN host galaxies and black hole activity

TL;DR

This study investigates how bars in spiral galaxies influence active galactic nuclei (AGN) properties, revealing that barred AGN hosts tend to have younger stars, higher nuclear activity, and increased black hole accretion rates compared to unbarred hosts.

Contribution

It provides a detailed comparison of barred and unbarred AGN host galaxies, highlighting the impact of bars on stellar populations and nuclear activity, using a large SDSS-DR7 sample with control matching.

Findings

Barred AGN hosts have a higher fraction of young stellar populations.

Barred AGN show a shift toward higher Lum[OIII] values.

Barred AGN exhibit higher black hole accretion rates.

Abstract

With the aim of assessing the effects of bars on active galactic nuclei (AGN), we present an analysis of host characteristics and nuclear activity of AGN galaxies with and without bars selected from the Sloan Digital Sky Survey Data Release 7 (SDSS-DR7). By visual inspection of SDSS images we classified the hosts of face-on AGN spiral galaxies brighter than g < 16.5 into barred or unbarred. With the purpose of providing an appropriate quantification of the effects of bars, we also constructed a suitable control sample of unbarred AGN galaxies with similar redshift, magnitude, morphology, bulge sizes and local environment distributions. We find that the bar fraction, with respect to the full sample of spiral face-on AGN host galaxies, is 28.5%, in good agreement with previous works. Barred AGN host galaxies show an excess of young stellar populations dominated by red u-r and g-r colors, with respect to the control sample, suggesting that bars produce an important effect on galaxy properties of AGN hosts. Regarding the nuclear activity distribution, we find that barred AGN galaxies show a shift toward higher Lum[OIII] values with respect to AGN without bars. In addition, we also find that this trend is more significant in less massive, younger stellar population and bluer AGN host galaxies. We found that the fraction of powerful AGN increase towards more massive hosts with bluer colors and younger stellar populations residing in denser environments. However, barred host AGN systematically show a higher fraction of powerful active nuclei galaxies with respect to the control sample. We also explored the accretion rate onto the central black holes finding that barred AGN show an excess of objects with high accretion rate values with respect to unbarred AGN galaxies.