The gas distribution and kinematics in the central region of the Seyfert 2 galaxy NGC 1125
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.
- Publication:
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Galaxy Evolution and Feedback across Different Environments
- Pub Date:
- 2021
- DOI:
- Bibcode:
- 2021IAUS..359..448M
- Keywords:
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- galaxies: Seyfert;
- galaxies: kinematics and dynamics;
- galaxies: individual (NGC 1125)