The impact of low luminosity AGN on their host galaxies: A radio and optical investigation of the kpc-scale outflow in MaNGA 1-166919

Abstract

One way an Active Galactic Nucleus (AGN) influences the evolution of their host galaxy is by generating a large-scale (kpc-scale) outflow. The content, energetics, and impact of such outflows depend on the properties of both the AGN and host galaxy, and understanding the relationship between them requires measuring the properties of all three. In this paper, we do so by analyzing recent radio and optical integral field unit (IFU) spectroscopic observations of MaNGA 1-166919. Our results indicate that the bi-conical outflow in this galaxy is powered by a low-luminosity, low-Eddington ratio AGN ejecting material that drives ~100-200 km/s shocks into the surrounding interstellar medium (ISM) -- producing the hot, ionized gas and relativistic particles associated with the observed outflow. The energetics of the relativistic and ionized gas material produced at this shock are comparable, and both the mass outflow and kinetic power of the ionized gas in this outflow are higher than other AGN with similar bolometric luminosities. Lastly, while the host galaxy's total star formation rate is comparable to that of other star-forming galaxies with a similar stellar mass, there is evidence that the outflow both suppresses and enhances star formation in its immediate surroundings.

arXiv comment29 pages, 28 figures, 11 tables, accepted by The Astrophysical Journal for publication

References in corpus (91)

• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• Astropy: A Community Python Package for Astronomy
• The Global Schmidt Law in Star Forming Galaxies
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• The Host Galaxies of AGN
• Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
• Star Formation in the Milky Way and Nearby Galaxies
• Theoretical Modeling of Starburst Galaxies
• The Host Galaxies and Classification of Active Galactic Nuclei
• Overview of the DESI Legacy Imaging Surveys
• Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
• The reversal of the star formation-density relation in the distant universe
• Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
• Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey
• Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations
• The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
• Information criteria for astrophysical model selection
• First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
• The MAPPINGS III Library of Fast Radiative Shock Models
• Calibrating Extinction-Free Star Formation Rate Diagnostics with 33GHz Free-Free Emission in NGC6946
• Present-Day Growth of Black Holes and Bulges: the SDSS Perspective
• Galaxy Zoo 1 : Data Release of Morphological Classifications for nearly 900,000 galaxies
• Powerful Outflows and Feedback from Active Galactic Nuclei
• On the fundamental dichotomy in the local radio-AGN population: accretion, evolution, and host galaxy properties
• A Catalog of Bulge+Disk Decompositions and Updated Photometry for 1.12 Million Galaxies in the Sloan Digital Sky Survey
• Dust-Corrected Star Formation Rates of Galaxies. II. Combinations of Ultraviolet and Infrared Tracers
• A comprehensive classification of galaxies in the SDSS: How to tell true from fake AGN?
• AGN wind scaling relations and the co-evolution of black holes and galaxies
• A multi-scale multi-frequency deconvolution algorithm for synthesis imaging in radio interferometry
• Dust Attenuation Curves in the Local Universe: Demographics and New Laws for Star-forming Galaxies and High-redshift Analogs
• Simulations of Ion Acceleration at Non-relativistic Shocks. I. Acceleration Efficiency
• Multi-Scale CLEAN deconvolution of radio synthesis images
• The physics of galactic winds driven by active galactic nuclei
• Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population
• The MaNGA Integral Field Unit Fiber Feed System for the Sloan 2.5 m Telescope
• The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey
• The SDSS-IV MaNGA Sample: Design, Optimization, and Usage Considerations
• SDSS IV MaNGA - Spatially resolved diagnostic diagrams: A proof that many galaxies are LIERs
• Quasar feedback and the origin of radio emission in radio-quiet quasars
• SDSS-IV MaNGA IFS Galaxy Survey --- Survey Design, Execution, and Initial Data Quality
• Evolutionary synthesis of galaxies at high spectral resolution with the code PEGASE-HR
• The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Overview
• The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library
• Feast and Famine: Regulation of Black Hole Growth in Low Redshift Galaxies
• The nature of LINER galaxies: Ubiquitous hot old stars and rare accreting black holes
• Driving Outflows with Relativistic Jets and the Dependence of AGN Feedback Efficiency on ISM Inhomogeneity
• SDSS-IV/MaNGA: Spectrophotometric Calibration Technique
• The Nature of LINER-like Emission in Red Galaxies
• Relativistic jet feedback III: feedback on gas disks
• Unification of the Fundamental Plane and Super-Massive Black Holes Masses
• Simultaneous Acceleration of Protons and Electrons at Nonrelativistic Quasiparallel Collisionless Shocks
• The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Emission-Line Modeling
• Accretion and star formation rates in low redshift type-II active galactic nuclei
• Accretion states and radio loudness in Active Galactic Nuclei: analogies with X-ray binaries
• Marvin: A Toolkit for Streamlined Access and Visualization of the SDSS-IV MaNGA Data Set
• Bursty stellar populations and obscured AGN in galaxy bulges
• But What About... Cosmic Rays, Magnetic Fields, Conduction, & Viscosity in Galaxy Formation
• Simulations and Theory of Ion Injection at Non-relativistic Collisionless Shocks
• Non-Thermal Electron Acceleration in Low Mach Number Collisionless Shocks. I. Particle Energy Spectra and Acceleration Mechanism
• Ionized outflows in local luminous AGN: what are the real densities and outflow rates?
• Ultra Fast Outflows: Galaxy-Scale Active Galactic Nucleus Feedback
• Discovering AGN-driven winds through their infrared emission: II. Mass outflow rate and energetics
• Upgrading electron temperature and electron density diagnostic diagrams of forbidden line emission
• The multiphase gas structure and kinematics in the circumnuclear region of NGC 5728
• The radio AGN population dichotomy: Green valley Seyferts versus red sequence low-excitation AGN
• Kinematics and stellar populations of the dwarf elliptical galaxy IC 3653
• Radiative cooling of swept up gas in AGN-driven galactic winds and its implications for molecular outflows
• AGN Feedback Compared: Jets versus Radiation
• Properties of the molecular gas in the fast outflow in the Seyfert galaxy IC 5063
• Deep Very Large Array observations of the merging cluster CIZA J2242.8+5301: continuum and spectral imaging
• The Prevalence of Gas Outflows in Type 2 AGNs. II. 3D Biconical Outflow Models
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• The Limited Impact of Outflows: Integral-Field Spectroscopy of 20 Local AGNs
• The Emission-Line Spectra of Major Mergers: Evidence for Shocked Outflows
• Winds as the origin of radio emission in $z=2.5$ radio-quiet extremely red quasars
• A Catalog of 406 AGNs in MaNGA: A Connection between Radio-mode AGN and Star Formation Quenching
• RCSED - A Value-Added Reference Catalog of Spectral Energy Distributions of 800,299 Galaxies in 11 Ultraviolet, Optical, and Near-Infrared Bands: Morphologies, Colors, Ionized Gas and Stellar Populations Properties
• Galactic disk winds driven by cosmic ray pressure
• Galaxy-scale AGN Feedback - Theory
• Unravelling the complex structure of AGN-driven outflows III. The outflow size-luminosity relation
• Unravelling the complex structure of AGN-driven outflows: II. Photoionization and energetics
• The Size-Luminosity Relationship of Quasar Narrow-Line Regions
• Evidence of ongoing AGN-driven feedback in a quiescent post starburst E+A galaxy
• Do Jet-Driven Shocks ionize the Narrow Line Regions of Seyfert Galaxies?
• Feedback by AGN Jets and Wide-Angle Winds on a Galactic Scale
• Feedback from low-luminosity radio galaxies: B2 0258+35
• Zooming into local active galactic nuclei: The power of combining SDSS-IV MaNGA with higher resolution integral field unit observations
• Quantifying the Thermal Sunyaev-Zel'dovich Effect and Excess Millimeter Emission in Quasar Environments
• Sensitive Radio Survey of Obscured Quasar Candidates
• FERMI-LAT Observations of Supernova Remnant G5.7-0.1, Believed to be Interacting with Molecular Clouds
• Dependence of optical Active Galactic Nuclei identification on stellar population models

Cited by in corpus (4)

• Radio Morphology of Red Geysers
• Stellar populations in local AGNs: evidence for enhanced star formation in the inner 100pc
• The [OIII] profiles of far-infrared active and non-active optically-selected green valley galaxies
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback