The Ultra-Fast Outflow of the Quasar PG 1211+143 as Viewed by Time-Averaged Chandra Grating Spectroscopy
arXiv:1712.07118 · doi:10.3847/1538-4357/aaa427
Abstract
We present a detailed X-ray spectral study of the quasar PG 1211+143 based on Chandra High Energy Transmission Grating Spectrometer (HETGS) observations collected in a multi-wavelength campaign with UV data using the Hubble Space Telescope Cosmic Origins Spectrograph (HST-COS) and radio bands using the Jansky Very Large Array (VLA). We constructed a multi-wavelength ionizing spectral energy distribution using these observations and archival infrared data to create XSTAR photoionization models specific to the PG 1211+143 flux behavior during the epoch of our observations. Our analysis of the Chandra-HETGS spectra yields complex absorption lines from H-like and He-like ions of Ne, Mg and Si which confirm the presence of an ultra-fast outflow (UFO) with a velocity ~ 17,300 km s (outflow redshift ~ 0.0561) in the rest frame of PG 1211+143. This absorber is well described by an ionization parameter ~ 2.9 erg s cm and column density ~ 21.5 cm. This corresponds to a stable region of the absorber's thermal stability curve, and furthermore its implied neutral hydrogen column is broadly consistent with a broad Ly absorption line at a mean outflow velocity of ~ 16,980 km s detected by our HST-COS observations. Our findings represent the first simultaneous detection of a UFO in both X-ray and UV observations. Our VLA observations provide evidence for an active jet in PG 1211+143, which may be connected to the X-ray and UV outflows; this possibility can be evaluated using very-long-baseline interferometric (VLBI) observations.
17 pages, 10 figures, published in The Astrophysical Journal, proof corrections applied
References in corpus (18)
- Space Telescope and Optical Reverberation Mapping Project. II. Swift and HST Reverberation Mapping of the Accretion Disk of NGC 5548
- Black hole feedback in the luminous quasar PDS 456
- The Low-z Intergalactic Medium. III. HI and Metal Absorbers at z<0.4
- Ultra-fast outflows in radio-loud active galactic nuclei
- The response of relativistic outflowing gas to the inner accretion disk of a black hole
- From ultraluminous X-ray sources to ultraluminous supersoft sources: NGC 55 ULX, the missing link
- 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?
- Confirming the high velocity outflow in PG 1211+143
- Relativistic blue- and red-shifted absorption lines in AGNs
- Revealing the ultra-fast outflow in IRAS 13224-3809 through spectral variability
- NuSTAR Reveals Relativistic Reflection But No Ultra-Fast Outflow In The Quasar PG 1211+143
- Intrinsic Absorption Properties in Active Galaxies Observed with the Far Ultraviolet Spectroscopic Explorer
- Is the X-ray spectrum of the narrow emission line QSO PG1211+143 defined by its energetic outflow?
- Discovery of an Ultraviolet Counterpart to an Ultra-Fast X-ray Outflow in the Quasar PG1211+143
- Testing relativistic reflection and resolving outflows in PG 1211+143 with XMM-Newton and NuSTAR
- MPI_XSTAR: MPI-based Parallelization of the XSTAR Photoionization Program
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- Monitoring AGNs with H Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars
- HST/COS Observations of Quasar Outflows in the 500-1050 Å Rest Frame: I. The Most Energetic Outflows in the Universe and Other Discoveries
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- Relativistic components of the Ultra-Fast Outflow in the Quasar PDS 456 from Chandra/HETGS, NuSTAR and XMM-Newton observations
- Discovery of an Ultraviolet Counterpart to an Ultra-Fast X-ray Outflow in the Quasar PG1211+143
- SDSS J075101.42+291419.1: A Super-Eddington Accreting Quasar with Extreme X-ray Variability
- HST/COS Observations of Quasar Outflows in the 500 -- 1050 Å Rest Frame: IV. The Largest Broad Absorption Line Acceleration
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- Galactic Winds across the Gas-Rich Merger Sequence: I. Highly Ionized N V and O VI Outflows in the QUEST Quasars
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- A deep, multi-epoch Chandra HETG study of the ionized outflow from NGC 4051
- Long-term X-ray Variability of the Symbiotic System RT Cru based on Chandra Spectroscopy
- A systematic study of the ultra-fast outflow responses to luminosity variations in active galactic nuclei
- Delving into the depths of NGC 3783 with XRISM III. Birth of an ultrafast outflow during a soft flare
- Constraining the geometry of AGN outflows with reflection spectroscopy
- A Search for H I Lyman Counterparts to Ultra-Fast X-ray Outflows
- X-ray Variability in the Symbiotic Binary RT Cru: Principal Component Analysis
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- Multiwavelength campaign on Mrk 509. XVI. Continued HST/COS monitoring of the far-ultraviolet spectrum
- Relativistic Reflection Modeling in AGN and Related Variability from PCA: A Brief Review
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- Disentangling the X-ray variability in the Lyman continuum emitter Haro 11
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- Accretion-disk reflection in the Seyfert 1 galaxy NGC 3783 as viewed by Chandra grating spectroscopy
- Winds Versus Jets in Active Galactic Nuclei