Location and energetics of the ultra-fast outflow in PG 1448+273
arXiv:2011.08212 · doi:10.1051/0004-6361/202039409
Abstract
Ultra-fast outflows (UFOs) play a key role in the AGN feedback mechanism. It is therefore important to fully characterize their location and energetics. We study the UFO in the latest XMM-Newton archival observation of the NLSy1 galaxy PG 1448+273 by means of a novel modeling tool, that is, the Wind in the Ionized Nuclear Environment model (WINE). Our detection of the UFO in PG 1448+273 is very robust. The outflowing material is highly ionized, erg s cm, has a large column density, cm, is ejected with a maximum velocity (90% c.l. errors), and attains an average velocity . WINE succeeds remarkably well to constrain a launching radius of from the black hole. We also derive a lower limit on both the opening angle of the wind () and the covering factor (). We find a mass outflow rate and a large instantaneous outflow kinetic power erg s = 24% = 18% ( errors). We find that a major error contribution on the energetics is due to , stressing the importance of an accurate determination through a proper spectral modeling, as done with WINE. Using 20 Swift (UVOT and XRT) observations and the simultaneous OM data from XMM-Newton, we also find that undergoes large variations, with a maximum excursion of , after the UFO is detected, leading to a remarkable X-ray weakness. This may point towards a starving of the inner accretion disk due to the removal of matter through the wind.
arXiv comment10 pages, 6 figures, 5 tables, accepted for publication in A&A
References in corpus (66)
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- The Swift X-ray Telescope
- The Swift Ultra-Violet/Optical Telescope
- A Catalog of Quasar Properties from SDSS DR7
- Spectral Energy Distributions and Multiwavelength Selection of Type 1 Quasars
- Powerful Outflows and Feedback from Active Galactic Nuclei
- The XMM-Newton Optical/UV Monitor Telescope
- Evidence for ultra-fast outflows in radio-quiet AGNs: I - detection and statistical incidence of Fe K-shell absorption lines
- Quasar Feedback: More Bang for Your Buck
- The physics of galactic winds driven by active galactic nuclei
- The XMM-Newton view of PG quasars I. X-ray continuum and absorption
- Measuring the broadband power spectra of active galactic nuclei with RXTE
- The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky Survey
- Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy
- Photoionization Modeling and the K Lines of Iron
- Unification of X-ray winds in Seyfert galaxies: from ultra-fast outflows to warm absorbers
- On the Nature of Soft X-ray Weak Quasi-Stellar Objects
- The multi-phase winds of Markarian 231: from the hot, nuclear, ultra-fast wind to the galaxy-scale, molecular outflow
- 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
- X-ray emission from radio-quiet quasars in the SDSS Early Data Release. The alpha_ox dependence upon UV luminosity
- CAIXA: a catalogue of AGN in the XMM-Newton archive III. Excess Variance Analysis
- Evidence for ultra-fast outflows in radio-quiet AGNs: III - location and energetics
- MHD Accretion-Disk Winds as X-ray Absorbers in AGNs
- Feedback from Mass Outflows in Nearby Active Galactic Nuclei I. UV and X-ray Absorbers
- The Dance of Heating and Cooling in Galaxy Clusters: 3D Simulations of Self-Regulated AGN Outflows
- Mechanical AGN Feedback: Controlling the Thermodynamical Evolution of Elliptical Galaxies
- Ultra-fast outflows in radio-loud active galactic nuclei
- The long term X-ray spectral variability of AGN
- Discovery of ultra-fast outflows in a sample of Broad Line Radio Galaxies observed with Suzaku
- AGN Feedback in Galaxy Groups: the Delicate Touch of Self-Regulated Outflows
- The Intrinsically X-ray Weak Quasar PHL 1811. I. X-ray Observations and Spectral Energy Distribution
- Host dynamics and origin of Palomar-Green QSOs
- Magnetically-Driven Accretion-Disk Winds and Ultra-Fast Outflows in PG1211+143
- The WISSH Quasars Project III. X-ray properties of hyper-luminous quasars
- Evidence for a radiatively driven disc-wind in PDS 456?
- Density Profiles in Seyfert Outflows
- Revealing the ultra-fast outflow in IRAS 13224-3809 through spectral variability
- Tracing the accretion history of supermassive Black Holes through X-ray variability: results from the Chandra Deep Field-South
- The most luminous blue quasars at . I. A tale of two X-ray populations
- Ensemble X-ray variability of Active Galactic Nuclei. II. Excess Variance and updated Structure Function
- Resolving the soft X-ray ultra fast outflow in PDS 456
- A long term study of AGN X-ray variability. Structure function analysis on a ROSAT-XMM quasar sample
- Variability and the X-ray/UV ratio of active galactic nuclei. II. Analysis of a low-redshift Swift sample
- Variability and the X-ray/UV ratio of Active Galactic Nuclei
- A study of the X-rayed outflow of APM 08279+5255 through photoionization codes
- The variable, fast soft X-ray wind in PG 1211+143
- Fe K Line Profile in Low-redshift Quasars: Average Shape and Eddington Ratio Dependence
- Physical Conditions in Ultra Fast Outflows in AGN
- Variable Nature of Magnetically-Driven Ultra-Fast Outflows
- HS 1700+6416: the first high redshift non lensed NAL-QSO showing variable high velocity outflows
- The X-ray/UV ratio in Active Galactic Nuclei: dispersion and variability
- On the importance of special relativistic effects in modelling ultra-fast outflows
- The XMM deep survey in the CDF-S. IX. An X-ray outflow in a luminous obscured quasar at z~1.6
- Discovery of an X-ray Quasar Wind Driving the Cold Gas Outflow in the Ultraluminous Infrared Galaxy IRAS F05189-2524
- Magnetized Disk-Winds in NGC 3783
- Relativistic components of the Ultra-Fast Outflow in the Quasar PDS 456 from Chandra/HETGS, NuSTAR and XMM-Newton observations
- The Wide-Angle Outflow of the Lensed z = 1.51 AGN HS 0810+2554
- Constraining the geometry of the nuclear wind in PDS 456 using a novel emission model
- PHL 1092 as a transient extreme X-ray weak quasar
- Quasar spectral variability from the XMM-Newton serendipitous source catalogue
- Magnified Views of the Ultrafast Outflow of the z = 1.51 AGN HS 0810+2554
- Yet another UFO in the X-ray spectrum of a high-z lensed QSO
- Detection of a variable ultra-fast outflow in the Narrow Line Seyfert 1 galaxy PG 1448+273
- Evidence for a clumpy disc-wind in the star forming Seyfert\,2 galaxy MCG--03--58--007
- Warm Absorber Diagnostics of AGN Dynamics
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- The intermediate-ionization lines as virial broadening estimators for Population A quasars
- The lively accretion disc in NGC 2992. III. Tentative evidence of rapid Ultra Fast Outflow variability
- Investigating the nuclear properties of highly accreting active galactic nuclei with XMM-Newton
- Star formation efficiency and AGN feedback in narrow-line Seyfert 1 galaxies with fast X-ray nuclear winds
- Ultra-high-energy cosmic rays from ultra-fast outflows of active galactic nuclei
- Rapid Variability of the accretion disk wind in the narrow line Seyfert 1, PG 1448+273
- Coordinated X-ray and UV absorption within the accretion disk wind of the active galactic nucleus PG 1126-041
- The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
- The XMM-Newton and NuSTAR view of IRASF11119+3257. I Detection of multiple UFO components and a very cold corona
- Effects of ultra-fast outflows on X-ray time lags in AGN
- X-ray Unveiling Events in a z~1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South
- Fast Outflowing Warm Absorbers in Narrow-Line Seyfert 1 Galaxy PG 1001+054 Revealed by HST/COS Spectra
- Winds Versus Jets in Active Galactic Nuclei
- X-HESS: a large sample of highly accreting serendipitous AGN under the XMM-Newton microscope