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Distance to Multiple Kinematic Components of Quasar Outflows: VLT Observations of QSO 2359-1241 and SDSS J0318-0600

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TLDR
In this article, the authors studied the multi-component outflow systems of two quasars exhibiting intrinsic Fe II absorption (QSO 2359-1241 and SDSS J0318-0600).
Abstract
Using high resolution VLT spectra, we study the multi-component outflow systems of two quasars exhibiting intrinsic Fe II absorption (QSO 2359-1241 and SDSS J0318-0600). From the extracted ionic column densities and using photoionization modeling we determine the gas density, total column density, and ionization parameter for several of the components. For each object the largest column density component is also the densest, and all other components have densities of roughly 1/4 of that of the main component. We demonstrate that all the absorbers lie roughly at the same distance from the source. Further, we calculate the total kinetic luminosities and mass outflow rates of all components and show that these quantities are dominated by the main absorption component.

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The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe

TL;DR: In this paper, the authors present a picture in which the population of active galactic nuclei (AGNs) can be divided into two distinct populations: radiative-mode AGNs are associated with black holes that produce radiant energy powered by accretion at rates in excess of ∼ 1% of the Eddington limit.
Journal ArticleDOI

Quasar feedback revealed by giant molecular outflows

TL;DR: In this article, the authors used the IRAM PdB Interferometer to observe the CO(1-0) transition in the closest quasar known, and they detected broad wings of the CO line, with velocities of up to 750 km/s-1 and spatially resolved on the kpc scale.
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AGN wind scaling relations and the co-evolution of black holes and galaxies

TL;DR: In this paper, the authors acknowledge support from the FP7 Career Integration Grant “eEASy” (CIG 321913), LZ acknowledges support from ASI/INAF grant I/037/12/0 and CF acknowledges funding from the European Union Horizon 2020 research and innovation programme under the Marie SklodowskaCurie grant agreement No 664931.
Journal ArticleDOI

The physics of galactic winds driven by active galactic nuclei

TL;DR: In this paper, it is shown that cooling of high-velocity shocked winds in AGN is in fact inefficient in a wide range of circumstances, including conditions relevant to ultraluminous infrared galaxies (ULIRGs), resulting in energy-conserving outflows.
Journal ArticleDOI

Quasar feedback revealed by giant molecular outflows

TL;DR: In this paper, the IRAM PdB Interferometer was used to detect broad wings of the CO line, with velocities up to 750 km/s and spatially resolved on the kpc scale.
References
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Journal ArticleDOI

CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra

TL;DR: In this article, the authors describe version 90 (C90) of the code, paying particular attention to changes in the atomic database and numerical methods that have affected predictions since the last publicly available version, C84.
Journal ArticleDOI

The quasar outflow contribution to agn feedback: vlt measurements of sdss j0318-0600*

TL;DR: In this article, high-resolution Very Large Telescope observations of the broad absorption line quasar SDSS J0318-0600 were used to extract accurate ionic column densities and determine an electron number density of ne = 103.3±0.2 cm−3 for the main outflow absorption component.
Journal ArticleDOI

Quasar Outflow Contribution to AGN Feedback: Observations of QSO SDSS J0838+2955

TL;DR: In this paper, a detailed analysis of the Astrophysical Research Consortium 3.5 m telescope spectrum of QSO SDSS J0838+2955 was presented, showing three broad absorption line (BAL) systems at 22,000, 13,000 and 4900 km s{sup -1} blueshifted from the systemic redshift of z = 2.043.
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