An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
arXiv:2306.03404 · doi:10.1093/mnras/stad1642
Abstract
While in massive galaxies active galactic nuclei (AGN) feedback plays an important role, the role of AGN feedback is still under debate in dwarf galaxies. With well spatially resolved data obtained from the Multi-Unit Spectroscopic Explorer (MUSE), we identify a spatially extended () and fast () AGN-driven outflow in a dwarf galaxy: SDSS J022849.51-090153.8 with that host an intermediate-mass black hole of and . Through the measurement of the rotation curve, we estimate the escape velocity of the halo and the ratio of the outflow velocity to the halo escape velocity to be , indicating that the outflow is capable of escaping not only the galaxy disk but the halo. The outflow size of our AGN is found to be larger than AGN in massive galaxies at the given AGN [O III] luminosity, while the size of the photo-ionized narrow-line region is comparable. These results suggest the important role of AGN feedback through outflows in dwarf galaxies when their central intermediate-mass black holes accrete at high-Eddington ratios.
arXiv comment12 pages, 2 tables, 12 figures, accepted for publication in MNRAS
References in corpus (86)
- A Universal Density Profile from Hierarchical Clustering
- Star Formation in Galaxies Along the Hubble Sequence
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- The Host Galaxies of AGN
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Theoretical Modeling of Starburst Galaxies
- The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- The Host Galaxies and Classification of Active Galactic Nuclei
- Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models
- First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- Galactic star formation and accretion histories from matching galaxies to dark matter haloes
- Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
- Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations
- Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
- The MUSE second-generation VLT instrument
- The Dust Opacity of Star-Forming Galaxies
- Evolutionary Stellar Population Synthesis with MILES. Part I: The Base Models and a New Line Index System
- Observational evidence for AGN feedback in early-type galaxies
- Automated data reduction workflows for astronomy
- Powerful Outflows and Feedback from Active Galactic Nuclei
- Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population
- The Horizon-AGN simulation: morphological diversity of galaxies promoted by AGN feedback
- Cool Outflows in Galaxies and their Implications
- High-resolution mass models of dwarf galaxies from LITTLE THINGS
- A New Sample of Low-mass Black Holes in Active Galaxies
- The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library
- Observations of Feedback from Radio-Quiet Quasars - II. Kinematics of Ionized Gas Nebulae
- The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0
- Properties of spherical galaxies and clusters with an NFW density profile
- The MOSDEF Survey: Electron Density and Ionization Parameter at
- Integral Field Spectroscopy of Massive, Kiloparsec-Scale Outflows in the Infrared-Luminous QSO Mrk 231
- Ionized gas outflows and global kinematics of low-z luminous star forming galaxies
- The Stellar Mass Tully-Fisher Relation to z=1.2 from AEGIS
- Deriving model-based T-consistent chemical abundances in ionised gaseous nebulae
- The bolometric luminosity of type 2 AGN from extinction-corrected [OIII]: no evidence for Eddington-limited sources
- Observations of Feedback from Radio-Quiet Quasars: I. Extents and Morphologies of Ionized Gas Nebulae
- The Prevalence of Gas Outflows in Type 2 AGNs
- Shaping the galaxy stellar mass function with supernova- and AGN-driven winds
- Extended Schmidt Law: Role Of Existing Stars In Current Star Formation
- Quasar-Mode Feedback in Nearby Type 1 Quasars: Ubiquitous Kiloparsec-Scale Outflows and Correlations with Black Hole Properties
- A Population of Bona Fide Intermediate Mass Black Holes Identified as Low Luminosity Active Galactic Nuclei
- The flux ratio of the [OIII] 5007,4959 lines in AGN: Comparison with theoretical calculations
- SDSS-IV MaNGA: Evidence of the importance of AGN feedback in low-mass galaxies
- MusE GAs FLOw and Wind (MEGAFLOW) III: galactic wind properties using background quasars
- Hubble Space Telescope Observations of Extended [O III] λ5007 Emission in Nearby QSO2s: New Constraints On AGN / Host Galaxy Interaction
- Multi-epoch Spectroscopy of Dwarf Galaxies with AGN Signatures: Identifying Sources with Persistent Broad H-alpha Emission
- IFU observations of luminous type II AGN - I. Evidence for ubiquitous winds
- MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
- Spatially resolved electron density in the Narrow Line Region of z<0.02 radio AGNs
- Breaking the Obscuring Screen: A Resolved Molecular Outflow in a Buried QSO
- AGN-Driven Outflows in Dwarf Galaxies
- AGN feedback in dwarf galaxies?
- A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
- Re-visiting the extended Schmidt law: the important role of existing stars in regulating star formation
- Fast and energetic AGN-driven outflows in simulated dwarf galaxies
- Tracing outflows in the AGN forbidden region with SINFONI
- The VLT SINFONI Mg ii Program for Line Emitters (SIMPLE) II: background quasars probing z 1 galactic winds
- Metallicity calibrations for diffuse ionised gas and low ionisation emission regions
- Exploring the limits of AGN feedback: black holes and the star formation histories of low-mass galaxies
- Unravelling the complex structure of AGN-driven outflows III. The outflow size-luminosity relation
- Properties of ionized outflows in MaNGA DR2 galaxies
- Intermediate-Mass Black Hole Growth and Feedback in Dwarf Galaxies at High Redshifts
- Chemical abundances of Seyfert 2 AGNs II. N2 metallicity calibration based on SDSS
- Spatially Extended NaI D Resonant Emission and Absorption in the Galactic Wind of the Nearby Infrared-Luminous Quasar F05189-2524
- Integral-Field Spectroscopy of Fast Outflows in Dwarf Galaxies with AGN
- A near-infrared study of the multi-phase outflow in the type-2 quasar J1509+0434
- Multi-phase outflows in post starburst E+A galaxies -- II. A direct connection between the neutral and ionized outflow phases
- A cuspy dark matter halo
- The spatial extension of extended narrow line regions in MaNGA AGN
- Discovering AGN-driven winds through their infrared emission: I. General method and wind location
- Hundreds of Low-Mass Active Galaxies in the Galaxy And Mass Assembly (GAMA) Survey
- . I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
- Near-Infrared Coronal Line Observations of Dwarf Galaxies hosting AGN-driven Outflows
- The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
- Half-Megasecond Chandra Spectral Imaging of the Hot Circumgalactic Nebula around Quasar Mrk 231
- Quasars Probing Quasars IX. The Kinematics of the Circumgalactic Medium Surrounding z ~ 2 Quasars
- EMPRESS. VI. Outflows Investigated in Low-Mass Galaxies with : Weak Feedback in Low-Mass Galaxies?
- Chemical abundances in the nuclear region of nearby galaxies from the Palomar Survey
- BH Accretion in Low-Mass Galaxies Since z~1
- AGN and Dwarf Galaxy Gas Kinematics
- Outflow kinematics manifested by the H-alpha line: gas outflows in Type 2 AGNs. IV
- Molecular Flows in Contemporary Active Galaxies and the Efficacy of Radio-Mechanical Feedback
- A universal relationship between stellar masses and binding energies of galaxies
- A 100-pc Scale, Fast and Dense Outflow in Narrow-Line Seyfert 1 Galaxy IRAS04576+0912
- AGN quenching in simulated dwarf galaxies