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Outflow signatures in Gemini GMOS-IFU observations of 5 nearby Seyfert 2 galaxies

Published online by Cambridge University Press:  29 March 2021

Izabel C. Freitas Open the ORCID record for Izabel C. Freitas [Opens in a new window] ,
Rogemar A. Riffel  and
Thaisa Storchi-Bergmann
Izabel C. Freitas
Affiliation:
Universidade Federal de Santa Maria, Colégio Politécnico, 97105-900, Santa Maria, RS, Brazil email: [email protected]
Rogemar A. Riffel
Affiliation:
Universidade Federal de Santa Maria, Departamento de Física, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil
Thaisa Storchi-Bergmann
Affiliation:
Instituto de Fsica, Universidade Federal do Rio Grande do Sul, Av. Bento Gonçalves 9500, 91501-970, Porto Alegre, RS, Brazil
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Abstract

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We use Gemini Multi-Object Spectrograph (GMOS) Integral Field Unit (IFU) observations of a sample of 5 bright nearby Seyfert galaxies to map their emission-line flux distributions and kinematics at a spatial resolution ranging from 110 to 280 pc. For all galaxies, the gas kinematics show two components: a rotation and an outflow component.

Keywords

galaxies: Seyfertgalaxies: kinematicsgalaxies: nuclei
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 274 - 276
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

References

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Storchi-Bergmann, T., et al. 1998, ApJ, 115, 909 10.1086/300242CrossRefGoogle Scholar