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.

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

Marconi, A.;Carniani, S.;Mannucci, F.
2021

Abstract

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.
2021
Settore FIS/05 - Astronomia e Astrofisica
Galaxy Evolution and Feedback across Different Environments
Bento Gonçalves, Brazil
2-6 marzo 2020
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments
Cambridge University Press
galaxies: individual (IC 5063; galaxies: ISM; galaxies: jets; galaxies: kinematics and dynamics; galaxies: Seyfert; NGC 5643); techniques: spectroscopic;
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11384/126402
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