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• W2914922334 endingPage "29" @default.
• W2914922334 startingPage "29" @default.
• W2914922334 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." @default.
• W2914922334 created "2019-02-21" @default.
• W2914922334 creator A5020887298 @default.
• W2914922334 creator A5037213463 @default.
• W2914922334 creator A5039769881 @default.
• W2914922334 creator A5074021272 @default.
• W2914922334 date "2019-02-28" @default.
• W2914922334 modified "2023-10-02" @default.
• W2914922334 title "Relativistic Components of the Ultra-fast Outflow in the Quasar PDS 456 from <i>Chandra</i>/HETGS, <i>NuSTAR</i>, and <i>XMM-Newton</i> Observations" @default.
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