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Feedback and star formation in AGNs

Published online by Cambridge University Press:  29 January 2021

Luis C. Ho
Luis C. Ho*
Affiliation:
Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China Department of Astronomy, School of Physics, Peking University, Beijing 100871, China
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Abstract

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I will describe a series of experiments designed to use measurements of the cold ISM content of quasars to constrain the effectiveness of AGN feedback. I will propose new star formation rate indicators and apply them to constrain the star formation rate in quasars.

Keywords

galaxies: activeactive: quasarsgalaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S356: Nuclear Activity in Galaxies Across Cosmic Time , October 2019 , pp. 223
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union