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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

A. C. Robleto-Orús
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Mexico
J. P. Torres-Papaqui
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Mexico
A. L. Longinotti
Affiliation:
Instituto Nacional de Astrofísica, Óptica y Electrónica, Mexico
R. A. Ortega-Minakata
Affiliation:
Instituto de Radioastronomía y Astrofísica, Univ. Nac. Aut. de México, Mexico
S. F. Sánchez
Affiliation:
Instituto de Astronomia, Universidad Nacional Autónoma de México, Mexico
Y. Ascasibar
Affiliation:
Departamento de Física Teórica, Universidad Autónoma de Madrid, Spain
E. Bellocchi
Affiliation:
Departamento de Física Teórica, Universidad Autónoma de Madrid, Spain
L. Galbany
Affiliation:
Departamento de Física Teórica y del Cosmos, Universidad de Granada, Spain
M. Chow-Martínez
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Mexico Instituto de Geología y Geofísica, Universidad Nacional Autónoma de Nicaragua, Nicaragua
J. J. Trejo-Alonso
Affiliation:
Facultad de Ingeniería, Universidad Autónoma de Querétaro, Mexico
A. Morales-Vargas
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Mexico
F. J. Romero-Cruz
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Mexico Tecnológico de Monterrey, Campus Irapuato, Mexico
K. A. Cutiva-Alvarez
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Mexico
R. Coziol
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Mexico
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Abstract

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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.

Type
Contributed Papers
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

References

Blustin, A. J., Kriss, G. A., Holczer, T., et al. 2007, A&A, 466, 1, 107118 Google Scholar
Bruzual, G. & Charlot, S. 2003, MNRAS, 344, 10001028 CrossRefGoogle Scholar
Cid Fernandes, R., Mateus, A., Sodré, L., et al. 2005, MNRAS, 358, 363378 CrossRefGoogle Scholar
Diaz-Santos, T., Alonso-Herrero, A., Colina, L., et al. 2007, ApJ, 661, 1, 149164 CrossRefGoogle Scholar
Freudling, W., Romaniello, M., Bramich, D. M., et al. 2013, A&A, 559, A96 Google Scholar
Genzel, R., Weitzel, L., Tacconi-Garman, Blietz, M., et al. 1995, ApJ, 444, 129–145CrossRefGoogle Scholar
Harrison, C. M., Alexander, D. M., Mullaney, J. R., et al. 2014, MNRAS, 441, 4, 33063347 CrossRefGoogle Scholar
Husemann, B., Jahnke, K., Sánchez, S. F., et al. 2014, MNRAS, 443, 1, 755783 CrossRefGoogle Scholar
Müller-Sánchez, F., Prieto, M. A., Hicks, E. K. S., et al. 2011, ApJ, 739, 2, 69 CrossRefGoogle Scholar
Weilbacher, P. I., Streicher, O., Urrutia, T., et al. 2014, ASP-CS, 485, 451 Google Scholar