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Gas flows in a changing-look AGN

Published online by Cambridge University Press:  29 March 2021

Sandra I. Raimundo Open the ORCID record for Sandra I. Raimundo [Opens in a new window]
Sandra I. Raimundo*
Affiliation:
DARK, Niels Bohr Institute, University of Copenhagen, Lyngbyvej 2, DK-2100 Copenhagen, Denmark email: sandra.raimundo@nbi.ku.dk
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Abstract

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The galaxy Mrk 590 is one of the few known ‘changing-look’ Active Galactic Nuclei (AGN) to have transitioned between states twice, having just increased its flux after a period of ˜10 years of low activity. In addition to the increase in flux, the optical broad emission lines have reappeared but show a different profile than what was observed before they disappeared. The gas motions in the host galaxy of this changing-look AGN show outflows and dynamical structures able to drive gas to the nucleus, suggesting an interplay between inflow and outflow in the centre of the galaxy.

Keywords

galaxies:activegalaxies:nucleigalaxies:individual(Mrk 590)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 334 - 338
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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