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A MUSE study of NGC 7469: Spatially resolved star-formation and AGN-driven outflows
Published online by Cambridge University Press: 29 March 2021
Abstract
NGC 7469 is a well-known type 1 AGN with a cirumnuclear star formation ring. It has previous detections of X-rays warm absorbers and an infrared biconical outflow. We analysed archival MUSE/VLT observations of this galaxy in order to look for an optical counterpart of these outflows. We report spatially resolved winds in the [O III] λ5007 emission line in two regimes: a high velocity regime possibly associated with the AGN and a slower one associated with the massive star formation of the ring. This slower regime is also detected with Hβ.
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- Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 291 - 294
- Copyright
- © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union