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Outflow signatures in Gemini GMOS-IFU observations of 5 nearby Seyfert 2 galaxies
Published online by Cambridge University Press: 29 March 2021
Abstract
We use Gemini Multi-Object Spectrograph (GMOS) Integral Field Unit (IFU) observations of a sample of 5 bright nearby Seyfert galaxies to map their emission-line flux distributions and kinematics at a spatial resolution ranging from 110 to 280 pc. For all galaxies, the gas kinematics show two components: a rotation and an outflow component.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 274 - 276
- Copyright
- © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union