Relativistic components of the Ultra-Fast Outflow in the Quasar PDS 456 from Chandra/HETGS, NuSTAR and XMM-Newton observations
arXiv:1901.06641 · doi:10.3847/1538-4357/ab0082
Abstract
We present the spectral analysis of Chandra/HETGS and NuSTAR observations of the quasar PDS 456 from 2015, and XMM-Newton and NuSTAR archival data from 2013-2014, together with Chandra/HETGS data from 2003. We analyzed these three different epochs in a consistent way, looking for absorption features corresponding to highly ionized blueshifted absorption lines from H-like and He-like ions of iron (and nickel), as well as of other elements (O, Ne, Si, and S) in the soft band. We confirm the presence of a persistent ultra-fast outflow (UFO) with a velocity of v_out=-0.24 - -0.29c, previously detected. We also report the detection of an additional faster component of the UFO with a relativistic velocity of v_out=-0.48c. We implemented photoionization modeling, using XSTAR analytic model warmabs, to characterize the physical properties of the different kinematic components of the ultra-fast outflow and of the partial covering absorber detected in PDS 456. These two relativistic components of the ultra-fast outflow observed in the three epochs analyzed in this paper are powerful enough to impact the host galaxy of PDS 456 through AGN feedback.
23 pages, 13 figures, 9 tables, accepted for publication in the Astrophysical Journal (ApJ) 2019 January 19
References in corpus (16)
- Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy
- Black hole feedback in the luminous quasar PDS 456
- A fast and long-lived outflow from the supermassive black hole in NGC 5548
- A Compton-thick Wind in the High Luminosity Quasar, PDS 456
- X-ray Absorption and Reflection in Active Galactic Nuclei
- Spectrum Synthesis Modeling of the X-ray Spectrum of GRO J1655-40 Taken During the 2005 Outburst
- Magnetically-Driven Accretion-Disk Winds and Ultra-Fast Outflows in PG1211+143
- Evidence for a radiatively driven disc-wind in PDS 456?
- The origin of ultra-fast outflows in AGN: Monte-Carlo simulations of the wind in PDS 456
- Line-driven disk wind model for ultra-fast outflows in active galactic nuclei -- Scaling with luminosity
- Does the X-ray outflow quasar PDS 456 have a UV outflow at 0.3c?
- The iron K feature in Narrow Line Seyfert 1's: evidence for a P Cygni profile?
- Physical Conditions in Ultra Fast Outflows in AGN
- Using principal component analysis to understand the variability of PDS 456
- X-ray flaring in PDS 456 observed in a high-flux state
- Testing relativistic reflection and resolving outflows in PG 1211+143 with XMM-Newton and NuSTAR
Cited by in corpus (10)
- Resolving the soft X-ray ultra fast outflow in PDS 456
- Location and energetics of the ultra-fast outflow in PG 1448+273
- The flaring X-ray corona in the quasar PDS 456
- Detection of a variable ultra-fast outflow in the Narrow Line Seyfert 1 galaxy PG 1448+273
- Linking the small scale relativistic winds and the large scale molecular outflows in the z = 1.51 lensed quasar HS 0810+2554
- X-raying winds in distant quasars: the first high-redshift wind duty cycle
- New radiative loss curve from updates to collisional excitation in the low-density, optically thin plasmas in SPEX
- Modelling X-ray RMS spectra II: the ultra-fast outflow of PDS 456
- Constraining X-ray Coronal Size with Transverse Motion of AGN Ultra-Fast Outflows
- Wind-luminosity evolution in NLS1 AGN 1H 0707-495