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arXiv · 2309.02491

BOSS Quasar Outflows Traced by C IV

Jarred Gillette·Fred Hamann
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Abstract

We investigate possible factors that drive fast quasar outflows using a sample of 39,249 quasars at median redshift $\langle z \rangle \approx$ 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 $\approx$ 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 Eddington ratios, and softer far-UV continuum (h$ν$ >24.6 eV). We find supporting evidence that radiative line-driving may generate extreme outflow velocities, influenced by multiple factors as suggested by the aforementioned correlations. This evidence highlights the importance of considering a multi-dimensional parameter space in future studies when analyzing large C IV blueshifts to determine the fundamental causes of outflows.

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Jarred Gillette, Fred Hamann. 2023-09-05. BOSS Quasar Outflows Traced by C IV. https://arxiv.org/abs/2309.02491

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