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A Separation of Systematic and Turbulent Motions in the Narrow-Line Region of NGC 4151

Published online by Cambridge University Press:  07 August 2017

Hartmut Schulz  and
Berto Boer
Hartmut Schulz
Affiliation:
Astronomical Institute of the Ruhr-University, Postfach 10 21 48, D-4630 Bochum 1, Federal Republic of Germany
Berto Boer
Affiliation:
Astronomical Institute of the Ruhr-University, Postfach 10 21 48, D-4630 Bochum 1, Federal Republic of Germany

Abstract

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Line profiles from the spatially resolved narrow-line region of NGC 4151 are separated into several bulk-motion components which show velocity dispersions two to three times larger than starburst nuclei with similar luminosity. The components are suggested to arise within the galactic disk and by filaments entrained in or situated along the shells of two super-bubbles. The large cone-like SW bubble is able to account for the SW soft-X ray excess and the hole in the NLR disk through which a UV-radiation cone emerges. The bubbles appear to be related to the nuclear radio source.

Type
Part 6: Velocity Fields, Kinematics, NL Profiles
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 352 - 354
Copyright
Copyright © Kluwer 1989 

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