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The gas distribution and kinematics in the central region of the Seyfert 2 galaxy NGC 1125
Published online by Cambridge University Press: 29 March 2021
Abstract
We present Gemini Near-Infrared Integral-Field Spectrograph (NIFS) observations of the inner 660 × 660 pc2 of the Seyfert 2 galaxy NGC 1125, which reveals that the emission-line profiles present two kinematic components: a narrow one (σ < 150 km s−1) due to emission of the gas in the disk and a broad component (σ > 150 km s−1) produced by a bipolar outflow, perpendicular to the galaxy’s disk.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 448 - 449
- Copyright
- © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union