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The gas distribution and kinematics in the central region of the Seyfert 2 galaxy NGC 1125

Published online by Cambridge University Press:  29 March 2021

Johan M. Marques
Affiliation:
Universidade Federal de Santa Maria, Departamento de Fsica, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil email: [email protected]
Rogemar A. Riffel
Affiliation:
Universidade Federal de Santa Maria, Departamento de Fsica, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil email: [email protected]
Thaisa Storchi-Bergmann
Affiliation:
Instituto de Fsica, Universidade Federal do Rio Grande do Sul, Av. Bento Gonçalves 9500, 91501-970 Porto Alegre, RS, Brazil
Rogério Riffel
Affiliation:
Instituto de Fsica, Universidade Federal do Rio Grande do Sul, Av. Bento Gonçalves 9500, 91501-970 Porto Alegre, RS, Brazil
Marlon R. Diniz
Affiliation:
Universidade Federal de Santa Maria, Departamento de Fsica, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil email: [email protected]
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Abstract

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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.

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

References

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