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Turbulence/outflows perpendicular to low-power jets in Seyfert galaxies

Published online by Cambridge University Press:  29 March 2021

Giacomo Venturi Open the ORCID record for Giacomo Venturi [Opens in a new window] ,
Alessandro Marconi ,
Matilde Mingozzi Open the ORCID record for Matilde Mingozzi [Opens in a new window] ,
Giovanni Cresci ,
Stefano Carniani Open the ORCID record for Stefano Carniani [Opens in a new window]  and
Filippo Mannucci
Giacomo Venturi
Affiliation:
Instituto de Astrofisica, Pontificia Universidad Católica de Chile, Avda. Vicuña Mackenna 4860, 8970117, Macul, Santiago, Chile email: gventuri@astro.puc.cl INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125, Firenze, Italy
Alessandro Marconi
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125, Firenze, Italy Dipartimento di Fisica e Astronomia, Università degli Studi di Firenze, Via G. Sansone 1, I-50019, Sesto Fiorentino, Firenze, Italy
Matilde Mingozzi
Affiliation:
INAF - Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122, Padova, Italy
Giovanni Cresci
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125, Firenze, Italy
Stefano Carniani
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125, Firenze, Italy Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy
Filippo Mannucci
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125, Firenze, Italy
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Abstract

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We present recent results from our MAGNUM survey of nearby active galactic nuclei (AGN), which exploits observations from the optical/near-IR integral field spectrograph MUSE at VLT. We detect strongly enhanced line widths in emission line maps of four galaxies perpendicularly to their low-power jets and AGN ionisation cones, indicative of turbulent/outflowing material. The observation of a similar phenomenon in other works suggests that it originates from an interaction mechanism between the jet and the galaxy disc through which it propagates.

Keywords

galaxies: jetsgalaxies: Seyfertgalaxies: individual (IC 5063, NGC 5643)galaxies: ISMgalaxies: kinematics and dynamicstechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 464 - 466
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

Footnotes

†

Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under program IDs 094.B-0321(A), 60.A-9339(A), 095.B-0532(A).

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