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A Magnetohydrodynamic Model of Galaxy Formation

Published online by Cambridge University Press:  12 April 2016

J. P. Sleath  and
A. H. Nelson
J. P. Sleath
Affiliation:
Department of Physics and Astronomy, University of Wales College of Cardiff, P.O. Box 913, Cardiff, CF2 3YB, U.K.
A. H. Nelson
Affiliation:
Department of Physics and Astronomy, University of Wales College of Cardiff, P.O. Box 913, Cardiff, CF2 3YB, U.K.

Abstract

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We present a full 3D model of galaxy formation, incorporating for the first time magnetohydrodynamical effects. By this means we hope to simulate the creation of active galactic nuclei, including jets. Preliminary results are encouraging.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 797 - 798
Copyright
Copyright © Astronomical Society of the Pacific 1997

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