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The role of AGN feedback in the baryon cycle at z ∼ 2

Published online by Cambridge University Press:  29 March 2021

Vincenzo Mainieri Open the ORCID record for Vincenzo Mainieri [Opens in a new window]
Vincenzo Mainieri*
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Strasse 2, Garching bei München, Germany
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Abstract

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In this proceeding I will summarize our on-going observational campaign to characterize Active Galactic Nuclei (AGN) driven ionized gas outflows at z ˜ 2 and assess their impact on galaxy evolution. The results are mostly derived from a recently completed SINFONI/VLT Large Programme named SUPER, conducted with Adaptive Optics to reach a spatial resolution of ˜2 kpc at z ˜ 2.

Keywords

galaxies: activegalaxies: ISMgalaxies: kinematics and dynamicsgalaxies: nuclei(galaxies:) quasars: emission lines
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 51 - 56
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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