A MUSE study of NGC 7469: Spatially resolved star-formation and AGN-driven outflows
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 spati...
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| Veröffentlicht in: | Proceedings of the International Astronomical Union 2020-03, Vol.15 (S359), p.291-294 |
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| creator | Robleto-Orús, A. C. Torres-Papaqui, J. P. Longinotti, A. L. Ortega-Minakata, R. A. Sánchez, S. F. Ascasibar, Y. Bellocchi, E. Galbany, L. Chow-Martínez, M. Trejo-Alonso, J. J. Morales-Vargas, A. Romero-Cruz, F. J. Cutiva-Alvarez, K. A. Coziol, R. |
| description | 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. |
| doi_str_mv | 10.1017/S1743921320001593 |
| format | Article |
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| subjects | Active galactic nuclei Astronomy Contributed Papers Galaxies Infrared analysis Massive stars Optical counterparts (astronomy) Outflow Star & galaxy formation Star formation |
| title | A MUSE study of NGC 7469: Spatially resolved star-formation and AGN-driven outflows |
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