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Radio-loud narrow-line Seyfert 1 galaxies with high-velocity outflows

Published online by Cambridge University Press:  07 March 2016

S. Komossa
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany email: skomossa@mpifr.de
D. Xu
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China
J. A. Zensus
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany email: skomossa@mpifr.de
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Abstract

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We have studied four radio-loud Narrow-line Seyfert 1 (NLS1) galaxies with extreme optical emission-line shifts, indicating radial outflow velocities of up 2450 km s−1. The shifts are accompanied by strong line broadening, up to 2270 km s−1 in [NeV]. A significant ionization stratification (higher line shift at higher ionization potential) of most ions implies that we see a large-scale wind rather than single, localized jet-cloud interactions. The observations are consistent with a scenario, where the signatures of outflows are maximized because of a pole-on view into the central engine of these radio-loud NLS1 galaxies.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., et al. 2009, ApJS, 182, 543Google Scholar
Fabian, A. 2012, ARAA, 50, 455Google Scholar
Komossa, S., Voges, W., Xu, D., et al. 2006, AJ, 132, 531Google Scholar
Komossa, S., Xu, D., Zhou, H., Storchi-Bergmann, T., & Binette, L. 2008, ApJ, 680, 926Google Scholar
Yuan, W., Zhou, H. Y., Komossa, S., et al. 2008, ApJ, 685, 801CrossRefGoogle Scholar