Host galaxy properties of changing-look AGNs revealed in the MaNGA survey

• Published in: Monthly notices of the Royal Astronomical Society Vol. 498; no. 3; pp. 3985 - 3994
• Main Authors: Yu, Xiaoling, Shi, Yong, Chen, Yanmei, Chen, Jianhang, Li, Songlin, Bing, Longji, Ge, Junqiang, Riffel, Rogemar A, Riffel, Rogério
• Format: Journal Article
• Language: English
• Published: Oxford University Press 01.11.2020
• Subjects: galaxies: Seyfert; galaxies: kinematics and dynamics; galaxies: nuclei; galaxies: active; galaxies: evolution
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/staa2627

ABSTRACT Changing-look active galactic nuclei (CL-AGNs) are a subset of AGNs in which the broad Balmer emission lines appear or disappear within a few years. We use the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey to identify five CL-AGNs. The 2D photometric and kinematic maps reveal common features as well as some unusual properties of CL-AGN hosts as compared to the AGN hosts in general. All MaNGA CL-AGNs reside in the star-forming main sequence, similar to MaNGA non-changing-look AGNs (NCL-AGNs). The $80 \pm 16{{\ \rm per\ cent}}$ of our CL-AGNs do possess pseudo-bulge features, and follow the overall NCL-AGN MBH–σ* relationship. The kinematic measurements indicate that they have similar distributions in the plane of angular momentum versus galaxy ellipticity. MaNGA CL-AGNs, however, show a higher, but not statistically significant ($20 \pm 16{{\ \rm per\ cent}}$) fraction of counter-rotating features compared to that ($1.84 \pm 0.61{{\ \rm per\ cent}}$) in general star formation population. In addition, MaNGA CL-AGNs favour more face-on (axial ratio > 0.7) than that of type I NCL-AGNs. These results suggest that host galaxies could play a role in the CL-AGN phenomenon.