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arXiv · 2003.08689

HST/COS Observations of Quasar Outflows in the 500 -- 1050 \AA\ Rest Frame: II The Most Energetic Quasar Outflow Measured to Date

Xinfeng Xu·Nahum Arav·Timothy Miller·Gerard A. Kriss·Rachel Plesha
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Abstract

We present a study of the BAL outflows seen in quasar SDSS J1042+1646 (z = 0.978) in the rest-frame 500 -- 1050 $\r{A}$ (EUV500) region. The results are based on the analysis of recent Hubble Space Telescope/Cosmic Origins Spectrograph observations. Five outflow systems are identified, where in total they include $\sim$70 outflow troughs from ionic transitions. These include the first non-solar detections from transitions of O V*, Ne V*, Ar VI, Ca VI, Ca VII, and Ca VIII. The appearance of very high-ionization species (e.g., Ne VIII, Na IX, and Mg X) in all outflows necessitates at least two-ionization phases for the observed outflows. We develop an interactive Synthetic Spectral Simulation method to fit the multitude of observed troughs. Detections of density sensitive troughs (e.g., S IV* $\lambda$ 657.32 $\r{A}$ and the O V* multiplet) allow us to determine the distance of the outflows ($R$) as well as their energetics. Two of the outflows are at $R$ $\simeq$ 800 pc and one is at $R$ $\simeq$ 15 pc. One of the outflows has the highest kinetic luminosity on record ($\dot{E_{k}}$ $ = 5\times 10^{46}$ erg s$^{-1}$), which is 20% of its Eddington luminosity. Such a large ratio suggests that this outflow can provide the energy needed for active galactic nucleus feedback mechanisms.

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Xinfeng Xu, Nahum Arav, Timothy Miller, Gerard A. Kriss, Rachel Plesha. 2020-03-19. HST/COS Observations of Quasar Outflows in the 500 -- 1050 \AA\ Rest Frame: II The Most Energetic Quasar Outflow Measured to Date. https://doi.org/10.3847/1538-4365/ab596a

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