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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

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