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 MBH–Mstellar 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.
Bohn, Thomas, et al. "A Near-infrared Look at AGN Feedback in Bulgeless Galaxies." The Astrophysical Journal, vol. 931, no. 1, May. 2022. https://doi.org/10.3847/1538-4357/ac6870
Bohn, Thomas, Canalizo, Gabriela, Satyapal, Shobita, & Sales, Laura V. (2022). A Near-infrared Look at AGN Feedback in Bulgeless Galaxies. The Astrophysical Journal, 931(1). https://doi.org/10.3847/1538-4357/ac6870
Bohn, Thomas, Canalizo, Gabriela, Satyapal, Shobita, et al., "A Near-infrared Look at AGN Feedback in Bulgeless Galaxies," The Astrophysical Journal 931, no. 1 (2022), https://doi.org/10.3847/1538-4357/ac6870
@article{osti_1983260,
author = {Bohn, Thomas and Canalizo, Gabriela and Satyapal, Shobita and Sales, Laura V.},
title = {A Near-infrared Look at AGN Feedback in Bulgeless Galaxies},
annote = {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 MBH–Mstellar 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.},
doi = {10.3847/1538-4357/ac6870},
url = {https://www.osti.gov/biblio/1983260},
journal = {The Astrophysical Journal},
issn = {ISSN 0004-637X},
number = {1},
volume = {931},
place = {United States},
publisher = {IOP Publishing},
year = {2022},
month = {05}}
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)
Sponsoring Organization:
Alfred P. Sloan Foundation; National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); USDOE Office of Science (SC)
OSTI ID:
1983260
Journal Information:
The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 931; ISSN 0004-637X