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Taurus Observations of the Emission-Line Velocity Field of Centaurus A (NGC 5128)

Published online by Cambridge University Press:  04 August 2017

Keith Taylor  and
Paul D. Atherton
Keith Taylor
Affiliation:
Anglo-Australian Observatory & Royal Greenwich Observatory
Paul D. Atherton
Affiliation:
Imperial College, London

Abstract

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Using TAURUS – an Imaging Fabry Perot system in conjunction with the IPCS on the AAT, we have studied the velocity field of the Ha emission line at a spatial resolution of 1.7″ over the dark lane structure of Centaurus A. The derived velocity field is quite symmetrical and strongly suggests that the emission line material is orbiting the elliptical component, as a warped disc.

Type
VI. Mergers
Information
Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 331 - 334
Copyright
Copyright © Reidel 1983 

References

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