The Ultraviolet-X-ray connection in AGN outflows
Elisa Costantini (SRON)

TL;DR
This paper reviews recent advances in understanding the physics of gas outflows from active galactic nuclei by analyzing combined ultraviolet and X-ray observations, highlighting their environmental impact.
Contribution
It synthesizes multiwavelength observational data to improve understanding of AGN outflows and their effects, offering a comprehensive overview of recent progress.
Findings
Enhanced understanding of AGN outflow mechanisms
Insights into the impact of outflows on galaxy evolution
Integration of UV and X-ray data improves modeling accuracy
Abstract
In this paper I review the recent progress in understanding the physics of the gas outflowing from active galactic nuclei and its impact on the surrounding environment, using the combined information provided by multiwavelength Ultraviolet-X-ray campaigns.
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