A Near-infrared Look at AGN Feedback in Bulgeless Galaxies

Bohn, Thomas; Canalizo, Gabriela; Satyapal, Shobita; Sales, Laura V.

doi:10.3847/1538-4357/ac6870

Title: A Near-infrared Look at AGN Feedback in Bulgeless Galaxies

Journal Article · Wed May 25 00:00:00 EDT 2022 · The Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/ac6870· OSTI ID:1983260

^[1];

^[2];

^[1]

Univ. of California, Riverside, CA (United States)
George Mason Univ., Fairfax, VA (United States)

While it is generally believed that supermassive black holes (SMBHs) lie in most galaxies with bulges, few SMBHs have been confirmed in bulgeless galaxies. Identifying such a population could provide important insights to the BH seed population and secular BH growth. To this end, we obtained near-infrared (NIR) spectroscopic observations of a sample of low-redshift bulgeless galaxies with mid-infrared colors suggestive of active galactic nuclei (AGNs). We find additional evidence of AGN activity (such as coronal lines and broad permitted lines) in 69% (9/13) of the sample, demonstrating that mid-infrared selection is a powerful tool to detect AGNs. More than half of the galaxies with confirmed AGN activity show fast outflows in [O III] in the optical and/or [Si vi] in the NIR, with the latter generally having much faster velocities that are also correlated to their spatial extent. We are also able to obtain virial BH masses for some targets and find they fall within the scatter of other late-type galaxies in the M_BH–M_stellar relation. The fact that they lack a significant bulge component indicates that secular processes, likely independent of major mergers, grew these BHs to supermassive sizes. Finally, we analyze the rotational gas kinematics and find two notable exceptions: two AGN hosts with outflows that appear to be rotating faster than expected. There is an indication that these two galaxies have stellar masses significantly lower than expected from their dark matter halo masses. This, combined with the observed AGN activity and strong gas outflows, may be evidence of the effects of AGN feedback.

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Research Organization:: US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE Office of Science (SC); National Science Foundation (NSF); Alfred P. Sloan Foundation; National Aeronautics and Space Administration (NASA)

Grant/Contract Number:: AST-1817233

OSTI ID:: 1983260

Journal Information:: The Astrophysical Journal, Vol. 931, Issue 1; ISSN 0004-637X

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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79 ASTRONOMY AND ASTROPHYSICS
Near infrared astronomy
Active galactic nuclei
Galaxy nuclei
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Seyfert galaxies
Galaxy bulges
Galaxy dark matter halos

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