BOSS Quasar Outflows Traced by C IV
Jarred Gillette, Fred Hamann

TL;DR
This study analyzes a large quasar sample to identify key factors driving high-velocity outflows, emphasizing the roles of Eddington ratios and UV continuum softness, and suggests radiative line-driving as a primary mechanism.
Contribution
It introduces a uniform re-measurement method for quasar redshifts based on Mg II, enabling exploration of unprecedented outflow velocities and correlations with physical quasar properties.
Findings
Higher C IV blueshifts correlate with broader, weaker emission profiles.
Faster outflows are associated with higher Eddington ratios and softer UV spectra.
Evidence supports radiative line-driving as a key mechanism for extreme outflows.
Abstract
We investigate possible factors that drive fast quasar outflows using a sample of 39,249 quasars at median redshift 2.17. Unique to this study, the quasar redshifts are re-measured based on the Mg II emission line, allowing for exploration of unprecedented outflow velocities (>6000 km/s) while maintaining statistical significance and uniformity. We measure reliable C IV blueshifts for 1178 quasars with velocities >2500 km/s. From those, 255(13) quasars have blueshifts above 4000(6000) km/s, with the highest C IV velocity 7000 km/s. Several correlations are observed, where higher C IV blueshifts in general are in quasars with broader, weaker C IV emission profiles, weak He II emission, larger Eddington ratios, and bluer UV continuum slope across the rest-frame UV to Near-IR. Analysis reveals two primary factors contributing to faster outflows: higher…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Astrophysical Phenomena and Observations
