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The impact of AGN on the life of their host galaxies at z ∼ 2

Published online by Cambridge University Press:  29 January 2021

Chiara Circosta
Chiara Circosta*
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany Dept. of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom email: [email protected]
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Abstract

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Feedback from active galactic nuclei (AGN) is thought to be key in shaping the life cycle of host galaxies by regulating star formation. Therefore, measuring the molecular gas reservoir out of which stars form is essential to understand the impact of AGN on star formation. In this talk I present an ongoing analysis to study the CO(J = 3−2) emission in a sample of 25 AGN at z ∼ 2 using ALMA observations. The CO properties of our AGN have been compared to normal (non-AGN) star-forming galaxies. The comparison between the two samples reveals that, on average, the CO luminosities of AGN at high stellar masses (log(M*/M⊙) > 11) are 0.5 dex lower than normal galaxies. We ascribe this difference to the AGN activity, which could be able to change the conditions of the gas through, e.g., excitation, heating or removal of CO.

Keywords

galaxies: activegalaxies: evolutionquasars: generalsurveysISM: jets and outflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S356: Nuclear Activity in Galaxies Across Cosmic Time , October 2019 , pp. 194 - 198
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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