Coordinated X-ray and UV absorption within the accretion disk wind of the active galactic nucleus PG 1126-041
arXiv:2306.05469 · doi:10.1051/0004-6361/202244270
Abstract
Accretion disk winds launched close to supermassive black holes (SMBHs) are a viable mechanism to provide feedback between the SMBH and the host galaxy. We aim to characterize the X-ray properties of the inner accretion disk wind of the nearby active galactic nucleus (AGN) PG 1126-041, and to study its connection with the ultraviolet (UV)-absorbing wind. We perform spectroscopic analysis of eight XMM-Newton observations of PG 1126-041 taken between 2004 and 2015, using both phenomenological models and the most advanced accretion disk wind models available. For half of the dataset, we can compare the X-ray analysis results with the results of quasi-simultaneous, high-resolution spectroscopic UV observations taken with the Cosmic Origins Spectrograph (COS) on board the Hubble Space Telescope. The X-ray spectra of PG 1126-041 are complex and absorbed by ionized material which is highly variable on multiple time scales, sometimes as short as 11 days. Accretion disk wind models can account for most of the X-ray spectral complexity of PG 1126-041, with the addition of massive clumps, represented by a partially covering absorber. Variations in column density ( cm) of the partially covering absorber drive the observed X-ray spectral variability of PG 1126-041. The absorption from the X-ray partially covering gas and from the blueshifted C IV troughs appear to vary in a coordinated way. The line of sight toward PG 1126-041 offers a privileged view through a highly dynamic nuclear wind originating on inner accretion disk scales, making the source a very promising candidate for future detailed studies of the physics of accretion disk winds around SMBHs.
arXiv comment24 pages, 13 figures, accepted for publication in Astronomy & Astrophysics
References in corpus (121)
- Planck 2015 results. XIII. Cosmological parameters
- On the Absorption of X-rays in the Interstellar Medium
- The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
- X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
- The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures
- Dynamics of line-driven disk winds in Active Galactic Nuclei
- Improved Reflection Models of Black-Hole Accretion Disks: Treating the Angular Distribution of X-rays
- Evidence for ultra-fast outflows in radio-quiet AGNs: I - detection and statistical incidence of Fe K-shell absorption lines
- AGN wind scaling relations and the co-evolution of black holes and galaxies
- Dynamics of Line-Driven Disk Winds in Active Galactic Nuclei II: Effects of Disk Radiation
- X-ray reflected spectra from accretion disk models. III. A complete grid of ionized reflection calculations
- The XMM-Newton view of PG quasars I. X-ray continuum and absorption
- A high velocity ionised outflow and XUV photosphere in the narrow emission line quasar PG1211+143
- The Spectral Energy Distributions of Low-Luminosity Active Galactic Nuclei
- A Catalog of Broad Absorption Line Quasars from the Sloan Digital Sky Survey Third Data Release
- A Catalog of Broad Absorption Line Quasars in Sloan Digital Sky Survey Data Release 5
- Simultaneous X-ray/optical/UV snapshots of active galactic nuclei from XMM-Newton: spectral energy distributions for the reverberation mapped sample
- A Model for the X-Ray and UV Emission from Seyfert Galaxies and Galactic Black Holes
- X-ray reflected spectra from accretion disk models. I. Constant density atmospheres
- On the Nature of Soft X-ray Weak Quasi-Stellar Objects
- A Massive X-Ray Outflow from the Quasar PDS 456
- Extreme X-ray spectral variability in the Seyfert 2 Galaxy NGC 1365
- Chandra Detects Relativistic Broad Absorption Lines from APM 08279+5255
- Black hole feedback in the luminous quasar PDS 456
- The Suzaku view of highly-ionised outflows in AGN: I - Statistical detection and global absorber properties
- A fast and long-lived outflow from the supermassive black hole in NGC 5548
- Evidence for ultra-fast outflows in radio-quiet AGNs: II - detailed photo-ionization modeling of Fe K-shell absorption lines
- First X-ray-Based Statistical Tests for Clumpy-Torus Models: Eclipse Events from 230 Years of Monitoring of Seyfert AGN
- XMM-NEWTON Reveals the Quasar Outflow in PG 1115+080
- Evidence for ultra-fast outflows in radio-quiet AGNs: III - location and energetics
- A Compton-thick Wind in the High Luminosity Quasar, PDS 456
- X-ray Spectroscopy of QSOs with Broad Ultraviolet Absorption Lines
- Ionized outflows from active galactic nuclei as the essential elements of feedback
- An Exploratory Chandra Survey of a Well-Defined Sample of 35 Large Bright Quasar Survey Broad Absorption Line Quasars
- On the Fraction of Quasars with Outflows
- A Chandra Survey of Broad Absorption Line Quasars
- A global view of the inner accretion and ejection flow around super massive black holes: radiation driven accretion disk winds in a physical context
- X-ray absorption by Broad Line Region Clouds in Mrk 766
- A combined Optical and X-ray Spectra Study for Type 1 AGN. III. Broadband SED Properties
- Variable partial covering and a relativistic iron line in NGC 1365
- How the X-ray spectrum of a Narrow-Line Seyfert 1 galaxy may be reflection dominated
- "Comets" orbiting a black hole
- Multi-dimensional modelling of X-ray spectra for AGN accretion-disk outflows III: application to a hydrodynamical simulation
- Variability in Quasar Broad Absorption Line Outflows I. Trends in the Short-Term versus Long-Term Data
- HST Observations of the Broad Absorption Line Quasar PG 0946+301
- A Suzaku survey of Fe K lines in Seyfert 1 AGN
- The Origins of AGN Obscuration: The 'Torus' as a Dynamical, Unstable Driver of Accretion
- The XMM-Newton long look of NGC 1365: uncovering of the obscured X-ray source
- Spectral Analysis of 1H0707-495 with XMM-Newton
- Host dynamics and origin of Palomar-Green QSOs
- Multi-dimensional modelling of X-ray spectra for AGN accretion-disk outflows
- Confirmation of and Variable Energy Injection by a Near-Relativistic Outflow in APM 08279+5255
- Extreme-Velocity Quasar Outflows and the Role of X-ray Shielding
- Chasing obscuration in type-I AGN: discovery of an eclipsing clumpy wind at the outer broad-line region of NGC 3783
- Heavy X-ray Absorption in Soft X-ray Weak Active Galactic Nuclei
- X-ray reflection in the Seyfert galaxy 1H0419-577 revealing strong relativistic effects in the vicinity of a Kerr black hole
- Weak Hard X-ray Emission from Broad Absorption Line Quasars: Evidence for Intrinsic X-ray Weakness
- XMM-Newton observations of the Narrow-Line Seyfert 1 galaxy Mrk 335 in an historical low X-ray flux state
- Suzaku observations of Mrk 335: Confronting partial covering and relativistic reflection
- The origin of ultra-fast outflows in AGN: Monte-Carlo simulations of the wind in PDS 456
- A disk wind interpretation of the strong Fe Kα features in 1H 0707-495
- The impact of accretion disk winds on the X-ray spectrum of AGN: Part 2 - XSCORT + Hydrodynamic Simulations
- Widespread, strong outflows in XQR-30 quasars at the Reionisation epoch
- Long-term spectral changes in the partial-covering candidate NLS1 1H 0707-495
- Relativistic blue- and red-shifted absorption lines in AGNs
- A blurred reflection interpretation for the intermediate flux state in Mrk 335
- Does the X-ray outflow quasar PDS 456 have a UV outflow at 0.3c?
- Short term X-ray spectral variability of the quasar PDS 456 observed in a low flux state
- The Extreme High-Velocity Outflow in Quasar PG0935+417
- A new relativistic component of the accretion disk wind in PDS 456
- Dramatic X-ray Spectral Variability of the Broad Absorption Line Quasar PG2112+059
- Results of Monitoring the Dramatically Variable C IV Mini-BAL System in the Quasar HS 1603+3820
- Variable X-ray absorption in the mini-BAL QSO PG 1126-041
- Galaxy-scale ionised winds driven by ultra-fast outflows in two nearby quasars
- Suzaku Observation of a Hard Excess in 1H 0419-577: Detection of a Compton-Thick Partial-Covering Absorber
- Line-driven disc wind in near-Eddington active galactic nuclei: decrease of mass accretion rate due to powerful outflow
- Supermassive Black Hole Winds in X-rays -- SUBWAYS. I. Ultra-fast outflows in QSOs beyond the local Universe
- UV line driven disc wind as the origin of ultrafast outflows in AGN
- The Multi-Layer Variable Absorbers in NGC 1365 Revealed by XMM-Newton and NuSTAR
- XMM-Newton Observations of Two BAL QSOs: Q1246-057 and SBS1542+541
- Discovery of a relativistic Fe line in PG 1425+267 with XMM--Newton and study of its short-timescale variability
- Multiphase AGN winds from X-ray irradiated disk atmospheres
- X-ray spectral variability in PG1535+547: the changing-look of a 'soft X-ray weak' AGN
- Anatomy of the AGN in NGC 5548: VII. Swift study of obscuration and broadband continuum variability
- The Long-Term X-Ray Variability of Broad Absorption Line Quasars
- Modeling the Fe K Line Profiles in Type I AGN with a Compton-Thick Disk Wind
- Discovery of a fast, broad, transient outflow in NGC 985
- A momentum conserving accretion disk wind in the narrow line Seyfert 1, I Zwicky 1
- Variability of the High Velocity Outflow in the Quasar PDS 456
- The Correlation between X-ray and UV Properties of BAL QSOs
- On the absorption of X-ray bright broad absorption line quasars
- On the diversity and complexity of absorption line profiles produced by outflows in Active Galactic Nuclei
- The nature of the extreme X-ray variability in the NLS1 1H 0707-495
- The fraction and kinematics of broad absorption line quasars across cosmic time
- HST/COS observations of the newly discovered obscuring outflow in NGC 3783
- Discovery of the Transition of a Mini-Broad Absorption Line into Broad Absorption in the SDSS Quasar J115122.14+020426.3
- Incoherent fast variability of X-ray obscurers. The case of NGC 3783
- Location and energetics of the ultra-fast outflow in PG 1448+273
- Constraining the geometry of the nuclear wind in PDS 456 using a novel emission model
- Interpretation of the X-ray Spectral Variation of 1H0707-495 with a Variable Double Partial Covering Model
- The X-ray Disk/Wind Degeneracy in AGN
- The WISSH quasars project X. Discovery of a multi-component and highly-variable UV ultra-fast outflow in a z=3.6 quasar
- A long hard look at the minimum state of PG 2112+059 with XMM-Newton
- Dynamical thermal instability in highly supersonic outflows
- Simultaneous XMM-\textit{Newton} and HST-COS observation of 1H0419-577: II. Broadband spectral modeling of a variable Seyfert galaxy
- Transient obscuration event captured in NGC 3227. I. Continuum model for the broadband spectral energy distribution
- NuSTAR Observations of Intrinsically X-ray Weak Quasar Candidates: An Obscuration-Only Scenario
- 10-Year Transformation of the Obscuring Wind in NGC 5548
- A New Emulated Monte Carlo Radiative Transfer Disk-Wind Model: X-Ray Accretion Disk-wind Emulator -- XRADE
- Resolving the X-ray obscuration in a low flux observation of the quasar PDS 456
- Obscuring clouds playing hide-and-seek in the Active Nucleus H0557-385
- Galactic Winds across the Gas-Rich Merger Sequence: I. Highly Ionized N V and O VI Outflows in the QUEST Quasars
- Dramatic changes in the observed velocity of the accretion disk wind in MCG-03-58-007 are revealed by XMM-Newton and NuSTAR
- Ionized Ultraviolet and Soft-X-ray Absorptions in the Low Redshift Active Galactic Nucleus PG1126-041
- On Synthetic Absorption Line Profiles of Thermally Driven Winds from Active Galactic Nuclei
- X-ray and multi-epoch optical/UV investigations of BAL to non-BAL quasar transformations
- Time variability of ultra-fast BAL outflows using SALT: C IV equivalent width analysis
- A Spectropolarimetric Test of the Structure of the Intrinsic Absorbers in the Quasar HS1603+3820
- Short time-scale X-ray spectral variability in the Seyfert 1 galaxy NGC 3783
- The X-Rays wind connection in PG 2112+059
- Unveiling the X-ray/UV properties of disk winds in active galactic nuclei using broad and mini-broad absorption line quasars